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Interstellar Dust and Circumstellar Dust Disks

  • Chapter
Interplanetary Dust

Part of the book series: Astronomy and Astrophysics Library ((AAL))

Abstract

Interstellar dust research belongs to the young branches of astrophysics. With the establishment of sensitive observational techniques in the astronomical infrared spectroscopy in the 1960s, diagnostic circumstellar and interstellar dust bands were detected and induced an explosive development of the whole field. In this context, the branch of solid-state astrophysics (synonymous to laboratory astrophysics) was founded. Special dust populations attributed to characteristic phases of the interstellar medium and to special circumstellar environments could be defined. Dust turned out to be the key to the understanding of the evolution of the interstellar medium and, closely connected with this, to the early and the late stages of stellar evolution. In this review, the population scheme is used for the division of the text to the main chapters. Evolutionary dust characteristics on the galactic scale and in the context of the formation of stars and planetary systems are stressed. Relations between interstellar and interplanetary solids are pointed out.

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References

  • Allamandola, L. J., Tielens, A. G. G. M., and Barker, J. R. 1987. Infrared absorption and emission characteristics of interstellar PAHs. In Interstellar Processes, eds. D. J. Hollenbach, H. A. Thronson (Dordrecht: Reidel), pp. 471–489.

    Google Scholar 

  • Allamandola, L. J., Sandford, S. A., Tielens, A. G. G. M., and Herbst, T. M. 1993. Diamonds in dense molecular clbuds: a challenge to the standard interstellar medium paradigm. Science, 260, pp. 64–66.

    ADS  Google Scholar 

  • Anders, E., and Zinner, E. 1993. Interstellar grains in primitive meteorites: Diamond, silicon carbide, and graphite. Meteoritics, 28, pp. 490–514.

    ADS  Google Scholar 

  • Andersen, A. C., Jäger, C., Mutschke, H., Braatz, A., Clément, D., Henning, Th., Jørgensen, U. G., and Ott, U. 1999. Infrared spectra of meteoritic SiC grains. Astron. Astrophys., 343, pp. 933–938.

    ADS  Google Scholar 

  • Anderson, C. M., Weitenbeck, A. J., Code, A. D., Nordsieck, K. H., Meade, M. R., Babler, B., Zellner, N. E. B., Bjorkman, K. S., Fox, K. G., and Johnson, J. J. 1996. Ultraviolet interstellar polarization of galactic starlight. I. Observations by the Wisconsin Ultraviolet Photo Polarimeter Experiment. Astron. J., 112, pp. 2726–2743.

    ADS  Google Scholar 

  • André, Ph. 1994. Disk-like structures around young stars. In Circumstellar Dust Disks and Planet Formation, eds. R. Ferlet and A. Vidal-Madjar (Gif sur Yvette: Editions Frontières), pp. 115–129.

    Google Scholar 

  • Artymowicz, P. 1994. Modeling and understanding the dust around beta Pictoris. In Circumstellar Dust Disks and Planet Formation, eds. R. Ferlet and A. Vidal-Madjar (Gif sur Yvette: Editions Frontières), pp. 47–65.

    Google Scholar 

  • Aumann, H. H., Gillett, F. C., Beichmann, C. A., de Jong, T., Houck, J. R., Low, F. J., Neugebauer, G., Walker, R. G., and Wesselius, P. R. 1984. Discovery of a shell around AIPha Lyrae. Astrophys. J., 278, pp. L23–L27.

    ADS  Google Scholar 

  • Baas, F., Grim, R. J. A., Geballe, T. R., Schutte, W., and Greenberg, J. M. 1988. The detection of solid methanol in W 33A. Dust in the Universe, eds. M. E. Bailey and D. A. Williams (Cambridge: Cambridge Univ. Press), pp. 55–60.

    Google Scholar 

  • Backman, D. E. and Paresce, F. 1993. Main-sequence stars with circumstellar solid material: the Vega phenomenon. In Protostars and Planets III, eds. E. H. Levy, J. I. Lunine, and M. S. Matthews (Tucson: Univ. Arizona Press), pp. 1253–1304.

    Google Scholar 

  • Backman, D. E., Werner, M. W., Rieke, G. H., and Van Cleve, J. E. 1997. Exploring planetary debris disks around solar-type stars. In From Stardust to Planetesimals, eds. Y. J. Pendleton and A. G. G. M. Tielens (San Francisco: Astron. Soc. Pacific), A. S. P. Conf. Ser. Vol. 122, pp. 49–66.

    Google Scholar 

  • Baggaley, W. J. 2000. Advanced Meteor Orbit Radar observations of interstellar meteoroids. J. Geophys. Res., 105 No. A5, pp. 10353–10362.

    ADS  Google Scholar 

  • Banhart, F. and Ajayan, P. M. 1996. Carbon onions as nanoscopic pressure cells for diamond formation. Nature, 382, pp. 433–435.

    ADS  Google Scholar 

  • Beckwith, S. V. W. 1994. Protoplanetary disks. In NATO Advanced Research Workshop on Theory of Accretion Disks - 2., eds. W. J. Duschl, J. Frank, F. Meyer, E. MeyerHofmeister, and W. Tscharnuter (Dordrecht: Kluwer Academ. Publ.), pp. 1–18.

    Google Scholar 

  • Beckwith, S. V. W., Sargent, A. I. 1991. Particle emissivity in circumstellar disks. Astrophys. J., 381, pp. 250–258.

    ADS  Google Scholar 

  • Beckwith, S. V. W., Sargent, A. I. 1996. Circumstellar disks and the search for neighboring planetary systems. Nature, 383, pp. 139–144.

    ADS  Google Scholar 

  • Begemann, B., Dorschner, J., Henning, T., Mutschke H., and Thamm, E. 1994. A laboratory approach to the interstellar sulfide dust problem. Astrophys. J., 423, pp. L71–L74.

    ADS  Google Scholar 

  • Begemann, B., Dorschner, J., Henning, Th., and Mutschke, H. 1996. Optical properties of glassy SiS2 and the 21 micron feature. Astrophys. J., 464, pp. L195–L198.

    ADS  Google Scholar 

  • Begemann, B., Dorschner, J., Henning, Th., Mutschke, H., Gurtler, Kömpe, C., Nass, R. 1997. Aluminum oxide and the opacity of oxygen-rich circumstellar dust in the 12-17-μm range. Astrophys. J., 476, pp. 199–208.

    ADS  Google Scholar 

  • Bernatowicz, T. J., Cowsik, R., Gibbons, P. C., Lodders, K., Fegley, Jr., B., Amari, S., and Lewis, R. S. 1996. Constraints on stellar grain formation from presolar graphite in the Murchison meteorite. Astrophys. J., 472, pp. 760–782.

    ADS  Google Scholar 

  • Beust, H., Lagrange, A.-M., Crawford, I. A., Goudard, C., Spyromilio, J., Vidal-Madjar, A. 1998. The β Pictoris circumstellar disk. XXV. The GaIl absorption lines and the Falling EvaporatiNg Bodies model revisited using UHRF observations. Astron. Astrophys., 338, pp 1015–1030.

    ADS  Google Scholar 

  • Biermann, P., and Harwitt, M. 1980. On the origin of the grain-size size spectrum of interstellar dust. Astrophys. J. Lett., 241, pp. L105–L107.

    ADS  Google Scholar 

  • Bless, R. C., and Savage, B. D. 1972. Ultraviolet photometry from the Orbiting Astronomical Observatory. II. Interstellar extinction. Astrophys. J., 171, pp. 293–308.

    ADS  Google Scholar 

  • Blitz, L. 1993. Giant molecular clouds. In Protostars & Planets III, edse E. H. Levy and J. I. Lunine (Tucson: Univ. Arizona Press), pp. 125–161.

    Google Scholar 

  • Blum, J., Wurm, G. 2000. Experiments on sticking, restructuring, and fragmentation of preplanetary dust aggregates. Icarus, 143, pp. 138–146.

    ADS  Google Scholar 

  • Blum, J., Wurm, G., Kempf, S. + 24 authors 2000. Growth and form of planetary seedlings: results from a microgravity aggregation experiment. Phys. Rev. Lett., 85, pp. 2426–2429.

    Google Scholar 

  • Bohren, C. F., and Huffman, D. R. 1983. Absorption and Scattering of Light by Small Particles (New York: Wiley).

    Google Scholar 

  • Boogert, A. C. A., Schutte, W. A., Tielens, A. G. G. M., et al. 1996. Solid methane toward deeply embedded protostars. Astron. A strophys., 315, pp. L377–L380.

    ADS  Google Scholar 

  • Boulanger,. F. 1994. Dust and gas in the infrared cirrus. In The First Symposium on the Infrared Cirrus and Diffuse Interstellar Clouds, eds. R. Cutri and W. B. Latter (San Francisco: Astron. Soc. Pacific), A. S. P. Conf. Ser., Vol. 58, pp. 101–114.

    Google Scholar 

  • Boulanger, F., Baud, B., and van Albada, G. D. 1985. Warm dust in the neutral interstellar medium. Astron. Astrophys., 144, pp. L9–L12.

    ADS  Google Scholar 

  • Boulanger, F., Prévot, M. L., and Gry, C. 1994. The contribution of small particles to the extinction curve. Astron. Astrophys., 284, pp. 956–970.

    ADS  Google Scholar 

  • Bouwman, J., de Koter, A., van den Ancker, M. E., and Waters, L. B. F. M. 2000. The composition of the circumstellar dust around the Herbig Ae stars AB Aur and HD 163296. Astron. Astrophys., 360, pp. 213–226.

    ADS  Google Scholar 

  • Braatz, A., Dorschner, J., Henning, Th., Jäger, C., and Ott, U. 1998. Infrared spectroscopy of presolar diamonds: The influence of chemical preparation. Meteoritics Planet. Sci., 33, p. A21.

    ADS  Google Scholar 

  • Braatz, A., Ott, U., Henning, Th., Jäger, C., and Jeschke, G. 2000. Infrared, ultraviolet, and electron paramagnetic resonance measurements on presolar diamonds: Implications for optical features and origin. Meteoritics Planet. Sci., 35, pp. 75–84.

    ADS  Google Scholar 

  • Bradley, J. P. 1996. The search for interstellar components in interplanetary dust. In Physics, Chemistry, and Dynamics of Interplanetary Dust: Proc. IAU Coll. 150, ed. B. Å. S. Gustafson (San Francisco: Astron. Soc. Pacific), A. S. P. Conf. Ser. Vol. 104, pp. 275–282.

    Google Scholar 

  • Bradley, J. P. 1999. Interstellar dust: evidence from interplanetary dust particles. In Formation and Evolution of Solids in Space, eds. J. M. Greenberg, A. Li (Dordrecht: Kluwer Academ. Publ.), NATO ASI Ser. C, Vol. 523, pp. 485–504.

    Google Scholar 

  • Bü;rki, P. R. 1996. Low-pressure formation routes for interstellar microdiamonds: chemical vapor deposition vs. homogeneous nucleation. Meteoritics, 31, pp. A24–A25.

    Google Scholar 

  • Buss Jr., R. H., Cohen, M., Tielens, A. G. G. M., Werner, M. W., Bregman, J. D., Witteborn, F. C., Rank, D., and Sandford, S.A. 1990. Hydrocarbon emission features in the infrared spectrum of warm supergiants. Astrophys. J., 365; pp. L23–L26.

    ADS  Google Scholar 

  • Butchart, I., McFadzean, A. D., Whittet, D. C. B., Geballe, T. R., Greenberg, J. M. 1986. Three micron spectroscopy of the galactic center source IRS7. Astron. Astrophys. Lett., 154, pp. L5–L7.

    ADS  Google Scholar 

  • Cardelli, J. A. 1994. Variability of interstellar extinction and its relationship to environment. In The First Symposium on the Infrared Cirrus and Diffuse Interstellar Clouds, eds. R. Cutri and W. B. Latter (San Francisco: Astron. Soc. Pacific), A. S. P. Conf. Ser. Vol. 58, pp. 24–33.

    Google Scholar 

  • Cardelli, J. A., Clayton, G. C., Mathis, J. S. 1988. The determination of ultraviolet extinction from the optical and near-infrared. Astrophys. J. Lett., 329, pp. L33–L37.

    ADS  Google Scholar 

  • Cesarsky, D., Jones, A. P., Lequeux, X., and Verstraete, L. 2000. Silicate emission in Orion. Astron. Astrophys., 358, pp. 708–716.

    ADS  Google Scholar 

  • Cherchneff, I., and Barker, J. R. 1992. Polycyclic aromatic hydrocarbons and molecular equilibria in carbon-rich stars. Astrophys. J., 394, pp. 703–716.

    ADS  Google Scholar 

  • Chiar, J. E., Tielens, A. G. G. M., Whittet, D. C. B., Schutte, W. A., Boogert, A. C. A., Lutz, D., van Dishoeck, E. F., and Bernstein, M. P. 2000. The composition and distribution of dust along the line of sight toward the Galactic center. Astrophys. J., 537, pp. 749–762.

    ADS  Google Scholar 

  • Chlewicki, G., and Laureijs, R. J. 1988. Model of grain properties based on IRAS observations. I. Evidence for new particle populations. Astron. Astrophys., 207, pp. L11–L14.

    ADS  Google Scholar 

  • Choi, B.-G., Huss, G. R., Wasserburg, G. J., Gallino, R. 1998. Presolar corundum and spinel in ordinary chondrites: origins from AGB stars and a supernova. Science, 282, pp. 1284–1289.

    ADS  Google Scholar 

  • Cohen, M., Tielens, A. G. G. M., and Bregman, J. D. 1989. Mid-infrared spectra of WC9 stars: The composition of circumstellar and interstellar dust. Astrophys. J. Lett., 344, pp. L13–L16.

    ADS  Google Scholar 

  • Colangeli, L., Mennella, V., Palumbo, P., and Rotundi, A. 1999. Cosmic dust and laboratory simulation: wishes, results and open problems. In Formation and Evolution of Solids in Space, eds. J. M. Greenberg, A. Li (Dordrecht: Kluwer Academ. Publ.), NATO ASI Ser. C, Vol. 523, pp. 203–228.

    Google Scholar 

  • Coulson, J. M., and Walther, D. M. 1995. SAO 206462 - a solar-type star with a dusty, organically rich environment. Mon. Not. Roy. Astron. Soc., 274, pp. 977–986.

    ADS  Google Scholar 

  • Coulson, I. M., Walther, D. M., and Dent, W. R. F. 1998. Infrared and submillimetre studies of Vega-excess stars. Monthly Not. R. Astron. Soc., 296, pp. 934–942.

    ADS  Google Scholar 

  • Cox, P. 1989. The line of sight towards AFGL 961: Detection of the librational band of water ice at 13.6 micron. Astron. Astrophys. Lett., 225, pp. L1–L4.

    ADS  Google Scholar 

  • Cox, P. 1993. Far-infrared spectroscopy of solid state features. In Astronomical Infrared Spectroscopy: Future Observational Directions, ed. S. Kwok (San Francisco, Astron. Soc. Pacific), A. S. P. Conf. Ser., Vol. 41, pp. 163–170.

    Google Scholar 

  • Cox, P., and Mezger, P. G. 1989. The galactic infrared/submillimeter dust radiation. Astron. Astrophys. Rev., 1, pp. 49–83.

    ADS  Google Scholar 

  • Crovisier, J., Leech, K., Bockelee-Morvan, D., Brooke, T. Y., Hanner, M. S., Altieri, B., Keller, H. U., and Lellouch, E. 1997. The spectrum of Comet Hale-Bopp (C/1995 01) observed with the Infrared Space Observatory at 2.9 astronomical units from the Sun. Science, 275, pp. 1904–1907.

    ADS  Google Scholar 

  • Dartois, E., Schutte, W., Geballe, T. R. Demyk, K., Ehrenfreund, P. d’Hendecourt, L. 1999. Methanol: the second most abundant ice species towards the high-mass protostars RAFGL7009S and W33A. Astron. Astrophys., 342, pp. L32–L35.

    ADS  Google Scholar 

  • Davis, L., and Greenstein, J. L. 1951. The polarization of starlight by aligned dust grains. Astrophys. J., 114, pp. 206–240.

    ADS  Google Scholar 

  • de Graauw, Th., Whittet, D. C. B., Gerakines, P. A. + 29 authors 1996. SWS observations of solid C02 in molecular clouds. Astron. A strophys., 315, pp. L345–L348.

    ADS  Google Scholar 

  • de Heer, W. A., and Ugarte, D. 1993. Carbon onions produced by heat treatment of carbon soot and their relation to the 217.5 nm interstellar absorption feature. Chem. Phys. Lett., 207, p. 480.

    ADS  Google Scholar 

  • Demyk, K., Jones, A. P., Dartois, E., Cox, P., and d’Hendecourt, L. 1999. The chemical composition of the silicate dust around RAFGL7009S and IRAS 19110+1045. Astron. Astrophys., 349, pp. 267–275.

    ADS  Google Scholar 

  • Desert, F.-X., Boulanger, F., and Puget, J. L. 1990. Interstellar dust models for extinction and emission. Astron. Astrophys., 237, pp. 215–236.

    ADS  Google Scholar 

  • d’Hendecourt, L. B., and Jourdain de Muizon, M. 1989. The discovery of interstellar carbon dioxide. Astron. Astrophys. Lett., 223, pp. L5–L8.

    ADS  Google Scholar 

  • d’Hendecourt, L. B. 1997. The PAH hypothesis: Infrared spectroscopic properties of PAHs. In Prom Stardust to Planetesimals, eds. Y. J. Pendleton and A. G. G. M. Tielens (San Francisco: Astron. Soc. Pacific), A. S. P. Conf. Ser., Vol. 122, pp. 129–145.

    Google Scholar 

  • Donn, B. 1968. Polycyclic hydrocarbons, Platt particles, and interstellar extinction. Astrophys. J. Lett., 152, pp. L129–L133.

    ADS  Google Scholar 

  • Dorschner, J. 1967. Theoretische Untersuchungen liber den interstellaren Staub. I. Vorschlag eines Staubmodells aus meteoritischen Silikaten. Astron. Nachr., 290, pp. 171–181.

    ADS  Google Scholar 

  • Dorschner, J. 1982. Interstellar grain size spectrum and circumstellar grain-grain collisions. Astrophys. Space Sci., 81, pp. 323–328.

    ADS  Google Scholar 

  • Dorschner, J. 1992. Interstellar dust, subject and agent of galactic evolution. Rev. Mod. Astron., 6, pp. 117–147.

    ADS  Google Scholar 

  • Dorschner, J. 1999. Stardust mineralogy: the laboratory approach. In Formation and EvoluINTERSTELLAR tion of Solids in Space, ed. J. M. Greenberg, A. Li (Dordrecht: Kluwer Academ. Publ.), NATO ASI Ser. C, Vol. 523, pp. 229–264.

    Google Scholar 

  • Dorschner, J., and Henning, Th. 1995. Dust metamorphosis in the Galaxy. Astron. Astrophys. Rev., 6, pp. 271–333.

    ADS  Google Scholar 

  • Dorschner, J., Friedemann, C., Gurtler, J., and Schielicke, R. 1984. A catalogue of equivalent widths ofthe interstellar 2000 Å band. Bull. InJ. Center Données Stellaires, 27, pp. 137–139.

    ADS  Google Scholar 

  • Dorschner, J., Begemann, B., Henning, Th., Jäger, C., and Mutschke, H. 1995. Steps toward interstellar silicate mineralogy. II. Study of Mg-Fe-silicate glasses of variable composition. Astron. Astrophys., 300, pp. 503–520.

    ADS  Google Scholar 

  • Draine, B. T. 1994. Dust in diffuse interstellar clouds. In The First Symposium on the Infrared Cirrus and Diffuse Interstellar Clouds, eds. R. Cutri and W. B. Latter (San Francisco: Astron. Soc. Pacific), A. S. P. Vol. 58, pp. 227–242.

    Google Scholar 

  • Draine, B. T., Lee, H. M. 1984. Optical properties of interstellar graphite and silicate grains. Astrophys. J., 285, pp. 89–108.

    ADS  Google Scholar 

  • Duley, W. W. 1988. Sharp emission lines from diamond dust in the Red Rectangle? Astrophys. Space Sci., 150, pp. 387–390.

    ADS  Google Scholar 

  • Duley, W. W. 1993. Carbonaceous grains. In Dust and Chemistry in Astronomy, eds. T. J. Millar and D. A. Williams (Bristol: Inst. Physics Publ.), pp. 71–101.

    Google Scholar 

  • Erickson, E. F., Knacke, R. F., Tokunaga, A. T., and Haas, M. R. 1981. The 45 micron H20 ice band in the Kleinmann-Low Nebula. Astrophys. J., 245, pp. 148–153.

    ADS  Google Scholar 

  • Fabian, D., Jäger, C., Henning, Th., Dorschner, J., and Mutschke, H. 2000. Steps toward interstellar silicate mineralogy. V. Thermal evolution of amorphous magnesium silicates and silica. Astron & Astrophys., 364, pp. 282–292.

    ADS  Google Scholar 

  • Fabian, D., Posch, Th., Mutschke, H., Kerschbaum, F. and Dorschner, J. 2001. Infrared optical properties of spinels. A study of the carrier of the 13, 17 and 32 p.m emission features observed in ISO-SWS spectra of oxygen-rich AGB stars. Astron. Astrophys., in press.

    Google Scholar 

  • Fajardo-Acosta, S. B., and Knacke, R. F. 1995. IRAS low resolution spectra with β Pictoristype silicate emission. Astron. Astrophys., 295, pp. 767–774.

    ADS  Google Scholar 

  • Ferrarotti, A., Gail, H.-P., Degiorgi, L., and Ott, H. R. 2000. FeSi as a possible new circumstellar dust component. Astron. Astrophys., 357, pp. L13–L16.

    ADS  Google Scholar 

  • Fischer, O., Henning, Th., and Yorke, H. W. 1995. Simulation of polarization maps. II. The circumstellar environments of pre-main sequence objects. Astron. Astrophys., 308, pp. 863–885.

    ADS  Google Scholar 

  • Fitzpatrick, E. L., and Massa, D. 1986. An analysis of the shapes of ultraviolet extinction curves. I. The 2175 Å bump. Astrophys. J., 307, pp. 286–294.

    ADS  Google Scholar 

  • Fitzpatrick, E. L., and Massa, D. 1990. An analysis of the shapes of ultraviolet extinction curves. III. An atlas of ultraviolet extinction curves. Astrophys. J. Suppl. Ser., 72, pp. 163-189.

    Google Scholar 

  • Freivogel, P., Fulara, J., Maier, J. P. 1994. Highly unsaturated hydrocarbons as potential carriers of some diffuse interstellar bands. Astrophys. J. Lett., 431, pp. L151–L154.

    ADS  Google Scholar 

  • Friedemann, Chr. 1969. Evolution of silicon carbide particles in the atmospheres of carbon stars. Physica, 41, pp. 139–143.

    ADS  Google Scholar 

  • Frisch, P. C., Dorschner, J. M., Geiss, J., Greenberg, J. M., Grün, E., Landgraf, M., Hoppe, P., Jones, A. P., Kratschmer, W., Linde, T. J., Morfill, G. E., Reach, W., Slavin, J. D., Svestka, J., Witt, A. N., and Zank, G. P. 1999. Dust in the local interstellar wind. Astrophys. J., 525, pp. 492–516.

    ADS  Google Scholar 

  • Gail, H.-P., Sedlymayr, E. 1998. Inorganic dust formation in astrophysical environments. In Chemistry and Physics of Molecules and Grains in Space, ed. P. Sarre (London: The Faraday Division of the Royal Society of Chemistry), Faraday Discussion, No. 109, p. 303.

    Google Scholar 

  • Geballe, T. R., Baas, F., Greenberg, J. M., Schutte, W. 1985. New infrared absorption features due to solid phase molecules containing sulfur. Astron. Astrophys. Lett., 146, pp. L6–L8.

    ADS  Google Scholar 

  • Geballe, T. R., Joblin, C., d’Hendecourt, L. B., Jourdain de Muizon, M., Tielens, A. G. G. M., and Leger, A. 1994. Detection of the overtone of the 3.3 micron emission feature in IRAS 21282 +5050. Astrophys. J. Lett., 434, pp. L15–L18.

    ADS  Google Scholar 

  • Geballe, T. R. 1997. Spectroscopy of the unidentified infrared emission bands. In From Stardust to Planetesimals, eds. Y. J. Pendleton and A. G. G. M. Tielens (San Francisco: Astron. Soc. Pacific), A. S. P. Conf. Ser., Vol. 122, pp. 119–128.

    Google Scholar 

  • Giard, M., Lamarre, J. M., Pajot, F., and Serra, G. 1994. The large scale distribution of PAHs in the Galaxy. Astron. Astrophys., 286, pp.:303–210.

    ADS  Google Scholar 

  • Gibb, E. L., Whittet, D. C. B., Schutte, W. A. + 8 authors 2000. An inventory of interstellar ices toward the embedded protostar W33A. Astrophys. J. Lett., 536, pp. 347–356.

    ADS  Google Scholar 

  • Gillett, F. C., and Forrest, W. J. 1973. Spectra of the Becklin-Neugebauer point source and the Kleinmann-Low nebula from 2.8 to 13.5 microns. Astrophys. J., 179, pp. 483–491.

    ADS  Google Scholar 

  • Glasse, A. C. H., Towlson, W. A., Aitken, D. K., and Roche, P.F. 1986. High-resolution infrared spectroscopy: A search for the 1l.52-pm graphite feature Mon. Not. Roy. Astron. Soc., 220, pp. 185–188.

    Google Scholar 

  • Goebel, J. H. 1993. SiS2 in circumstellar shells. Astron. Astrophys., 278, pp. 226–230.

    ADS  Google Scholar 

  • Goebel, J. H., and Moseley, S.H. 1985. MgS grain component in circumstellar shells. Astrophys. J. Lett., 290, pp. L35–L39.

    ADS  Google Scholar 

  • Gordon, K. D., Witt, A. N., Rudy, R. J., Puetter, R. C., Lynch, D. K., Mazuk, S., Misselt, K. A., Clayton, G. C. and Smith, T. L. 2000. Dust emission features in NGC 7023 between 0.35 and 2.5 11m: Extended Red Emission (0.7 μm) and two new emission features (1.15 and 1.5 μm). Astrophys. J., in press.

    Google Scholar 

  • Gordon, K. D., Witt, A. N.., and Friedmann, B. C. 1998. Detection of extended red emission in the diffuse interstellar medium. Astrophys. J., 498, pp. 522–540.

    ADS  Google Scholar 

  • Gorti, U., Bhatt, H. C. 1993. Anomalous dust in the environment of Herbig Ae/Be star. Astron. Astrophys., 270, pp. 426–431.

    ADS  Google Scholar 

  • Grady, C. A., Sitko, M. L., Bjorkman, K. S., Pérez, M. R., Lynch, D. K., Russell, R. W., Hanner, M. S. 1997. The star-grazing extrasolar comets in the HD 100546 system. Astrophys. J., 483, pp. 449–456.

    ADS  Google Scholar 

  • Greenberg, J. M. 1973. Some scattering problems of interstellar grains. In Interstellar Dust and Related Topics: Proc. IAU Symp., 52, eds. J. M. Greenberg and H.C. van de Hulst (Dordrecht: Reidel), pp. 3–9.

    Google Scholar 

  • Greenberg, J. M. 1984. Evolution of interstellar grains. Occasional Rep. Royal Obs. Edinburgh, 12, pp. 1–25.

    ADS  Google Scholar 

  • Greenberg, J. M. 1989. The core-mantle model of interstellar grains and the cosmic dust connection In Interstellar Dust: Proc. IA U Symp. 135, eds. L. J. Allamandola and A. G. G. M. Tielens (Dordrecht: Kluwer Academ. Publ.), pp. 345–355.

    Google Scholar 

  • Greenberg, J. M. and Li, A. 1995. What are the true astronomical silicates? Astron. Astrophys., 309, pp. 258–266.

    ADS  Google Scholar 

  • Grim, R. J. A. and Greenberg, J. M. 1987. Ions in grain mantles: The 4.62 micron absorption by OCN- in W33A. Astrophys. J. Lett., 321, pp. L91–L96.

    ADS  Google Scholar 

  • Grim, R. J. A., Baas, F., Geballe, T. R., Greenberg, J. M., and Schutte, W. 1991. Detection of solid methanol in W33A. Astron. Astrophys., 243, pp. 473–477.

    ADS  Google Scholar 

  • Grün, E., Gustafson, B., Mann, I., Baguhl, M., Morfill, G. E., Staubach, P., Taylor, A., and Zook, H. A. 1994. Interstellar dust in the heliosphere. Astron. Astrophys., 286, pp. 915–924.

    ADS  Google Scholar 

  • Grün, E., Landgraf, M., Horányi, M., Kissel, J., Kruger, H., Srama, R., Svedhem, H., and Withnell, P. 2000. Techniques for galactic dust measurement in the heliosphere. J. Geophys. Res., 105 No. A5, pp. 10403–10410.

    ADS  Google Scholar 

  • Gurtler, J., Henning, Th., Dorschner, J. 1989. Properties of circumstellar silicate dust (Review). Astron. Nachr., 310, pp. 319–327.

    ADS  Google Scholar 

  • Gurtler, J., Henning, Th., Kömpe, C., Pfau, W., Krätschmer, W., and Lemke, D. 1996. Detection of an absorption feature at the position of the 4.27-μm band of solid CO2. Astron. Astrophys., 315, pp. L189–L192.

    ADS  Google Scholar 

  • Gurtler, J., Schreyer, K., Henning, Th., Lemke, D., and Pfau, W. 1999. Infrared spectra of young stars in Chamaeleon. Astron. Astrophys., 346, pp. 205–210.

    ADS  Google Scholar 

  • Guillois, O., Ledoux, G.. and Reynaud, C. 1999. Diamond infrared emission bands in circumstellar media. Astrophys. J. Lett., 521, pp. L133–L136.

    ADS  Google Scholar 

  • Hall, J. S. 1949. Observations of the polarized light from stars. Science, 109, p. 166.

    ADS  Google Scholar 

  • Hallenbeck, S. L., Nuth, J. A., and Daukantas, P. L. 1998. Mid-infrared spectral evolution of amorphous magnesium silicate smokes annealed in vacuum: comparison to cometary spectra. Icarus, 131, pp. 198–209.

    ADS  Google Scholar 

  • Hanner, M. S. 1995. Dust around young stars: How related to solar system dust? Highlights of Astronomy, 10, pp. 351–392.

    ADS  Google Scholar 

  • Hanner, M. S. 1999. The silicate material in comets. Space Sci. Rev., 90, pp. 99–108.

    ADS  Google Scholar 

  • Hanner, M. S., Lynch, D. K., and Russell, R. W. 1994a. The 8-13 micron spectra of comets and the composition of silicate grains. Astrophys. J., 425, pp. 274–285.

    ADS  Google Scholar 

  • Hanner, M. S., Brooke, T. Y., and Tokunaga, A. T. 1994b. Silicates and aromatic hydrocarbons in the 10 micron spectrum of the Taurus dark cloud Elias 1. Astron. J. Lett., 433, pp. L97–100.

    ADS  Google Scholar 

  • Hanner, M. S., Brooke, T. Y., and Tokunaga, A. T. 1998. 8-13 micron spectroscopy of young stars. Astrophys. J., 502, pp. 871–882.

    ADS  Google Scholar 

  • Hecht, J. H. 1991. The nature of the dust around R Coronae Borealis stars: Isolated amorphous carbon or graphite fractals? Astrophys. J, 367, pp. 635–640.

    ADS  Google Scholar 

  • Henning, Th. 1996. Circumstellar dust around young stars. In The Cosmic Dust Connection, ed. J. M. Greenberg (Dordrecht: Kluwer), NATO ASI Ser. C, Vol. 487, pp. 399–412.

    Google Scholar 

  • Henning, Th., and Salama, F. 1998. Carbon in the universe. Science, 282, pp. 2204–2210.

    ADS  Google Scholar 

  • Henning, Th., and Schnaiter, M. 1999. Carbon - From space to laboratory. In Laboratory Astrophysics and Space Research, eds. P. Ehrenfreund, C. Kraft, H. Kochan, and V. Pirronello (Dordrecht: Kluwer), pp. 249–277.

    Google Scholar 

  • Henning, Th., Dorschner, J., and Gurtler, J. 1989. Size distribution of dust grains - a problem of self-similarity? In Interstellar Dust: Contributed Papers, NASA CP 3036, p. 395.

    Google Scholar 

  • Henning, Th., Begemann, B., Mutschke, H., and Dorschner, J. 1995. Optical properties of oxide dust grains. Astron. Astrophys. Suppl. Ser., 112, pp. 143–149.

    ADS  Google Scholar 

  • Herbig, G. H. 1995. The diffuse interstellar bands. Annu. Rev. Astrophys., 33, pp. 19–73.

    ADS  Google Scholar 

  • Hill, H. G. M., Jones, A. P., d’Hendecourt, L. B. 1998. Diamonds in carbon-rich protoplanetary nebulae. Astron. Astrophys., 336, pp. L41–L44.

    ADS  Google Scholar 

  • Hiltner, W. A. 1949. On the presence of polarization in the continuum radiation of stars. Astrophys. J., 109, pp. 471–478.

    ADS  Google Scholar 

  • Hoffmeister, C. 1929. On the heliocentric velocity of meteors. Astrophys. J., 69, pp. 159–167.

    ADS  Google Scholar 

  • Hoffmeister, C. 1931. Zur physikalischen Theorie der Sternschnuppen. Astron. Nachr., 241, pp. 1–8.

    ADS  Google Scholar 

  • Hong, S. S., and Greenberg, J. M. 1978. On the size distribution of interstellar grains. Astron. Astrophys., 70, pp. 695–699.

    ADS  Google Scholar 

  • Hoppe, P. and Ott, U. 1997. Mainstream silicon carbide grains from Meteorites. In Astrophysical Implications of the Laboratory Study of Presolar Material, eds. T. J. Bernatowicz and E. Zinner, AIP Conf. Ser. Proceed., 402, pp. 27–58.

    Google Scholar 

  • Hoppe, P. and Zinner, E. 2000. Presolar dust grains from meteorites and their stellar sources. J. Geophys. Res., 105 No. A5, pp. 10371–10385.

    ADS  Google Scholar 

  • Hoyle, F., and Wickramasinghe, N. C. 1962. On graphite particles as interstellar grains. Mon. Not. Roy. Astron. Soc., 124, pp. 417–433.

    ADS  Google Scholar 

  • Hron, J., Aringer, B., and Kerschbaum 1997. Semiregular variables of types SRa and SRb. Silicate dust emission features. Astron. Astrophys., 322, pp. 280–290.

    ADS  Google Scholar 

  • Jäger, C., Mutschke, H., Begemann, B., Dorschner, J., and Henning, Th. 1994. Steps toward interstellar silicate mineralogy. I. Laboratory results of a silicate glass of mean cosmic composition. Astron. Astrophys., 292, pp. 641–655.

    ADS  Google Scholar 

  • Jäger, C., Mutschke, H., and Henning, Th. 1998a. Optical properties of carbonaceous dust analogs. Astron. Astrophys., 332, pp. 291–299.

    ADS  Google Scholar 

  • Jäger, C., Molster, F., Dorschner, J., Henning, Th., Mutschke, H., and Waters, L. B. F. M. 1998b. Steps toward interstellar silicate mineralogy. IV. The crystalline revolution. Astron. Astrophys., 339, pp. 904–916.

    ADS  Google Scholar 

  • Jenniskens, P., and Desert, F.-X. 1993. A survey of diffuse interstellar bands (3800-8680 Å) Astron. Astrophys. Suppl. Ser., 106, pp. 39–78.

    ADS  Google Scholar 

  • Jenniskens, P., and Greenberg, J. M. 1993. Environment dependence of interstellar extinction curves. Astron. Astrophys., 274, pp. 439–450.

    ADS  Google Scholar 

  • Jones, A. P. 1997. The lifecycle of interstellar dust. In Prom Stardust to Planetesimals, eds. Y. J. Pendleton and A. G. G. M. Tielens (San Francisco: Astron. Soc. Pacific), A. S. P. Conf. Ser., Vol. 122, pp. 97–106.

    Google Scholar 

  • Jones, A. P., and Williams, D. A. 1987. Interplanetary material as a guide to the composition of interstellar grains. Mon. Not. R. Astron. Soc., 224, pp. 473–479.

    ADS  Google Scholar 

  • Jones, A. P., and Tielens, A. G. G. M. 1994. Interstellar dust - physical processes. In The Gold Universe, eds. Th. Montmerle, Ch. J. Lada, I. F. Mirabel, and J. Trãn Thanh Vãn (Gif sur Yvette: Editions Frontières), pp. 35–44.

    Google Scholar 

  • Jones, A. P., Tielens, A. G. G. M., and Hollenbach, D. J. 1996 Grain shattering in shocks: the interstellar grain size distribution. Astrophys. J., 469, pp. 740–764.

    ADS  Google Scholar 

  • Kamijo, F. 1963. A theoretical study of the long period variable stars. III. Formation of solid or liquid particles in the circumstellar envelope. Publ. Astron. Soc. Japan, 15, pp. 440–448.

    ADS  Google Scholar 

  • Keller, L. P., Bradley, J. P., Bouwman, J., Molster, F. J., Waters, L. B. F. M., Flynn, G. J., Henning, T., and Mutschke, H. 2000. Sulfides in interplanetary dust particles: a possible match to the 23 /Lm feature detected by the Infrared Space Observatory. Abstracts 31st Annual LPS conference, Abstract No. 1860.

    Google Scholar 

  • Kim, S.-H., and Martin, P. G. 1995. The size distribution of interstellar dust particles as determined from polarization: spheroids. Astrophys. J., 444, pp. 293–305.

    ADS  Google Scholar 

  • Kim, S.-H., Martin, P. G., and Hendry, P. D. 1994. The size distribution of interstellar dust particles as determined from extinction. Astrophys. J., 422, pp. 164–175.

    ADS  Google Scholar 

  • Knacke, R. F., Fajardo-Acosta, S. B., Telesco, C. M., Hackwell, J. A., Lynch, D. K., and Russell, R. W. 1993. The silicates in the disk of β Pictoris. Astrophys. J., 418, pp. 440–450.

    ADS  Google Scholar 

  • Koike, C., Kimura, S., Kaito, C., Suto, H., Shibai, H., Nagata, T., Tanabe, T., and Saito, Y. 1995. Correlation between the spectral index and the degree of crystallization of carbon and graphite grains. Astrophys. J., 446, pp. 902–906.

    ADS  Google Scholar 

  • Koike, C., Wickramasinghe, N. C., Kano, N., Yamakoshi, K., Yamamoto, T., Kaito, C., Kimura, S., and Okuda, H. 1995. The infrared spectra of diamond-Like residues from the Allende meteorite. Monthly Not. R. Astron. Soc., 277, pp. 986–994.

    ADS  Google Scholar 

  • Kwok, S., Volk, K. M., Hrivnak, B. J. 1989. A 21 micron emission feature in four protoplanetary nebulae. Astrophys. J., 345, pp. L51–L54.

    ADS  Google Scholar 

  • Lada, E. A., Strom, K. M., and Myers, P. C. 1993. Environments of star formation: relationship between molecular clouds, dense cores, and young stars. In Protostars β Planets III, eds. E. H. Levy and J. I. Lunine (Tucson: Univ. Arizona Press), pp. 245–277.

    Google Scholar 

  • Lacy, J. H., Baas, F., Allamandola, L. J., Perssons, S. E. McGregor, P. J., Lonsdale, C. J., Geballe, T. R., van de Bult, C. E. P. 1984. 4.6 micron absorption features due to solid phase CO and cyano group molecules toward compact infrared sources. Astrophys. J., 276, pp. 533–543.

    ADS  Google Scholar 

  • Lacy, J. H., Faraji, H., Sandford, S. A., and Allamandola, L. J. 1998. Unraveling the 10 micron “silicate” feature of protostars: the detection of frozen interstellar ammonia. Astrophys. J., 501, pp. L105–L109.

    ADS  Google Scholar 

  • Lagage, P.O., and Pantin, E. 1994. Probing dust around main-sequence stars with TIMMI. The Messenger, 75, pp. 24–26.

    ADS  Google Scholar 

  • Landgraf, M., Baggaley, W. J., Grün, E., Kruger, H., and Linkert, G 2000. Aspects of the mass distribution of interstellar grains in the solar system from in-situ measurements. J. Geophys. Res., 105 No. A5, pp. 10343–10352.

    ADS  Google Scholar 

  • Lanz, T., Heap, S. R., and Hubeny, I. 1995. HST/GHRS observations of the j3 Pictoris system: basic parameters and the age of the system. Astrophys. J., 447, pp. L41–L44.

    ADS  Google Scholar 

  • Larson, H. P., Davis, D. S., Black, J. H., and Fink, U. 1985. Interstellar absorption features toward the compact infrared source W33A. Astrophys. J., 299, pp. 873–880.

    ADS  Google Scholar 

  • Ledoux, G., Ehbrecht, M., Guillois, O., Huisken, F., Kohn, B., Laguna, M. A., Nenner, I., Paillard, V., Papoular, R., Porterat D., and Reynaud, C. 1998. Silicon as a candidate carrier for ERE. Astron. Astrophys., 333, pp. L39–L42.

    ADS  Google Scholar 

  • Lenzuni, P., Gail, H.-P., and Henning, Th. 1995. Dust evaporation in protostellar cores. Astrophys. J., 447, pp. 848–862.

    ADS  Google Scholar 

  • Li, A., and Greenberg, J. M. 1997. A unified model of interstellar dust. Astron. Astrophys., 323, pp. 566–584.

    ADS  Google Scholar 

  • Lillie, C. F., and Witt, A. N. 1976. Ultraviolet photometry from the Orbiting Astronomical Observatory. XXV. Diffuse galactic light in the 1500-4200 Å region and the scattering properties of interstellar dust grains. Astrophys. J., 208, pp. 64–74.

    ADS  Google Scholar 

  • Linde, T.J., and Gombosi, T.I. 2000. Interstellar dust filtration at the heliospheric interfase. J. Geophys. Res., 105, pp. 10411–10417.

    ADS  Google Scholar 

  • Loys de Cheseaux, J. P. 1744. Traite des Gometes.

    Google Scholar 

  • Lutz, D., Feuchtgruber, H., Genzel, R., + 11 authors 1996. SWS observations of the Galactic center. Astron. Astrophys., 315, pp. L269–L272.

    ADS  Google Scholar 

  • Lynds, B. T. 1968. Dark nebulae. In Stars and Stellar Systems., Vol. VII, eds. B. M. Middlehurst and L. H. Aller (Chicago: Univ. Chicago Press), pp. 119–139.

    Google Scholar 

  • Malfait, K., Bogaert, E., and Waelkens, C. 1998a. An ultraviolet, optical and infrared study of Herbig Ae/Be stars. Astron. Astrophys., 331, pp. 211–223.

    ADS  Google Scholar 

  • Malfait, K., Waelkens, C., Waters, L. B. F. M, Vandenbussche, B., Huygen, E., and De Graauw, M. S. 1998b. The spectrum of the young star HDI00546 observed with the Infrared Space Observatory. Astron. Astrophys., 332, pp. L25–L28.

    ADS  Google Scholar 

  • Maifait, K., Waelkens, C., Bouwman, J., De Koter, A., and Waters, L. B. F. M. 1999. The ISO spectrum of the young star HD142527. Astron. Astrophys., 345, pp. 181–186.

    ADS  Google Scholar 

  • Martin, P. G. 1989. Linear and circular polarization in the diffuse interstellar medium. In Interstellar Dust: Proc. IAU Symp., 135, eds. L. J. Allamandola and A. G. G. M. Tielens (Dordrecht: Kluwer Academ. Publ.), pp. 55–65.

    Google Scholar 

  • Martin, P. G., and Whittet, D. C. B. 1990. Interstellar extinction and polarization in the infrared. Astrophys. J., 357, pp. 113–124.

    ADS  Google Scholar 

  • Mathis, J. S. 1993. Observations and theories of interstellar dust. Rep. Prog. Phys., 56, pp. 605–652.

    ADS  Google Scholar 

  • Mathis, J. 1996. Dust models with tight abundance constraints. Astrophys. J., 472, pp. 643–655.

    ADS  Google Scholar 

  • Mathis, J. 1998. The near-infrared interstellar silicate bands and grain theories. Astrophys. J., 497, pp. 824–832.

    ADS  Google Scholar 

  • Mathis, J. S., and Whiffen, G. 1989. Composite interstellar grains. Astrophys. J., 341, pp. 808–822.

    ADS  Google Scholar 

  • Mathis, J. S., Rumpl, W., Nordsieck, K. H. 1977. The size distribution of interstellar grains. Astrophys. J., 217, pp. 425–433.

    ADS  Google Scholar 

  • Mattila, K., Lemke, D., Haikala, L. K., Laureijs, R.J., Léger, A., Lehtinen, K., Leinert, Ch., and Mezger, P. G. 1996. Spectrophotometry of UIR bands in the diffuse emission of the galactic disk. Astron. Astrophys., 315, pp. L353–L356.

    ADS  Google Scholar 

  • McDonnell, J. A. M. 1988. Solar system dust as a guide to interstellar matter. In Dust in the Universe, eds. M.E. Bailey and D.A. Williams (Cambridge: Cambridge University Press), pp. 169–18l.

    Google Scholar 

  • McKee, C. F., and Ostriker, J. P. 1977. A theory of the interstellar medium: Three components regulated by supernova explosions in a inhomogeneous substrate. Astrophys. J., 218, pp. 148–169.

    ADS  Google Scholar 

  • Mennella, V., Colangeli, L., Blanco, A., Bussoletti, E., Fonti, S., Palumbo, P., and Mertins, H. C. 1995a. A dehydrogenation study of cosmic carbon analogue grains Astrophys. J., 444, pp. 288–292.

    Google Scholar 

  • Mennella, V., Colangeli, L., Bussoletti, E., Monaco G., Palumbo, P., and Rotundi, A. 1995b. On the electronic structure of small carbon grains of astrophysical interest. Astrophys. J. Suppl. Ser., 100, pp. 149–157.

    ADS  Google Scholar 

  • Men’shchikov, A. B., Henning, Th., and Fischer, O. 1999. Self-consistent model of the dusty torus around HL Tauri. Astrophys. J., 519, pp. 257–278.

    ADS  Google Scholar 

  • Molster, F. J. 2000. Crystalline silicates in circumstellar dust shells. Ph. D. Thesis, University of Amsterdam.

    Google Scholar 

  • Molster, F. J., Waters, L. B. F. M., Trams, N., + 8 authors 1999a. The composition and nature of the dust shell surrounding the binary AFGL4106. Astron. Astrophys., 350, pp. 163–180.

    ADS  Google Scholar 

  • Molster, F. J., Yamamura, I., Waters, L. B. F. M., + 9 authors 1999b. Low-temperature crystallization of silicate dust in circumstellar disks. Nature, 401, p. 563.

    ADS  Google Scholar 

  • Mutschke, H., Dorschner, J., Henning, Th., Jäger, C., and Ott, U. 1995. Facts and artifacts in interstellar diamond spectra. Astrophys. J. Lett., 454, pp. L157–L160.

    ADS  Google Scholar 

  • Mutschke, H., Begemann, B., Dorschner, J., and Henning, Th., 1998. Steps toward interstellar silicate mineralogy. III. The role of aluminium in stardust silicates. Astron. Astrophys., 333, pp. 188–198.

    ADS  Google Scholar 

  • Mutschke, H., Andersen, A. C., Clément, D., Henning, Th., and Peiter, G. 1999. Infrared properties of SiC particles. Astron. Astrophys., 345, pp. 187–202.

    ADS  Google Scholar 

  • Ney, E. P. 1977. Star dust. Science, 195, pp. 541–546.

    ADS  Google Scholar 

  • Nittler, L. R. 1997. Presolar oxide grains in meteorites. In Astrophysical Implications of the Laboratory Study of Presolar Material, eds. T. J. Bernatowicz and E. Zinner, AIP Conf. Ser. Proceed., 402, pp. 59–82.

    Google Scholar 

  • Nittler, L. R, Hoppe, P., Alexander, C. M. O’D., + 7 authors 1995 Silicon nitride from supernovae. Astrophys. J. Lett., 453, pp. L25–L28.

    Google Scholar 

  • Nuth, J. A. 1996. Grain formation and metamorphism. In The Cosmic Dust Connection, ed. J.M. Greenberg (Dordrecht: Kluwer Academ. Publ.), pp. 205–221.

    Google Scholar 

  • Nuth, J. A., Moseley, S. H., Silverberg, R. F., Goebel, J. H., and Moore, W. H. 1985. Laboratory infrared spectra of predicted condensates in carbon-rich stars. Astrophys. J., 290, pp. L41–L43.

    ADS  Google Scholar 

  • Nuth III, J. A., Hallenbeck, S. L., and Rietmeijer, F. J. M. 1999. Interstellar and interplanetary grains. Recent developments and new opportunities for experimental chemistry. In Laboratory Astrophysics and Space Research, eds. P. Ehrenfreund, C. Kraft, H. Kochan, and V. Pirronello (Dordrecht: Kluwer), pp. 143–182.

    Google Scholar 

  • O’Dell, C. R, and Wen, Z. 1994. Post refurbishment mission Hubble Space Telescope images of the core of the Orion nebula: Proplyds, Herbig-Haro objects, and measurements of a circumstellar disk. Astrophys. J., 436, pp. 194–202.

    ADS  Google Scholar 

  • Olbers, W. 1823. Über die Durchsichtigkeit des Weltraumes. In Wilhelm Gibers. Sein Leben und seine Werke, Bd. 1, ed. C. Schilling (Berlin: Julius Springer 1894), pp. 133–141.

    Google Scholar 

  • Olnon, F. M., Raimond, E. (eds.) 1986. IRAS catalogues and atlases. Atlas of low-resolution spectra. Astron. Astrophys. Suppl. Ser., 65, pp. 607–1065.

    Google Scholar 

  • Omont, A., Moseley, S. H., Forveille, T., Glaccum, W. J., Harvey, P. M., Likkel, L., Loewenstein, R F., and Lisse, C. M. 1990. Observations of 40-70 micron bands of ice in IRAS 09371 +1212 and other stars. Astrophys. J. Lett., 355, pp. L27–L30.

    ADS  Google Scholar 

  • Omont, A., Moseley, S. H., Cox, P., + 8 authors 1995. The 30 micron emission band in carbon-rich pre-planetary nebulae. Astrophys. J., 454, pp. 819–825.

    ADS  Google Scholar 

  • Onaka, T., de Jong, T., and Willems, F. J. 1989. A study of M Mira variables based on IRAS LRS observations. I. Dust formation in the circumstellar shell. Astron. Astrophys., 218, pp. 169–179.

    ADS  Google Scholar 

  • Oort, J. H., van de Hulst, H. C. 1946. Gas and smoke in interstellar space. Bull. Astron. Inst. Netherlands, 10, pp. 187–204.

    ADS  Google Scholar 

  • Öpik, E. 1929. Zur Theorie der Variation der Sternschnuppenhäufigkeit. Astron. Nachr., 235, pp. 265–268.

    ADS  Google Scholar 

  • Öpik, E. 1931. On the physical interpretation of color-excess in early type stars. Harvard Cire., No. 359.

    Google Scholar 

  • Ossenkopf, V. 1993. Dust coagulation in dense molecular clouds: the formation of fluffy aggregates. Astron. Astrophys., 280, pp. 617–646.

    ADS  Google Scholar 

  • Padgett, D. L., Brandner, W., Stapelfeldt, K. R., Strom, S. E., Terebey, S., and Koerner, D. 1999. Hubble Space Telescope/NICMOS imaging of disk and envelopes around very young stars. Astron. J., 117, pp. 1490–1504.

    ADS  Google Scholar 

  • Palumbo, M. E., Tielens, A. G. G. M., Tokunaga, A. T. 1995. Solid carbonyl sulphide (OCS) in W33A. Astrophys. J., 449, pp. 674–680.

    ADS  Google Scholar 

  • Pendleton, Y. J., and Chiar, J. E. 1997. The nature and evolution of interstellar organics. In Prom Stardust to Planetesimals, eds. Y. J. Pendleton and A. G. G. M. Tielens (San Francisco: Astron. Soc. Pacific), A. S. P. Conf. Ser., Vol. 122, pp. 179–200.

    Google Scholar 

  • Posch, Th., Kerschbaum, F., Mutschke, H., Fabian, D., Dorschner, J., and Hron, J. 1999. On the origin of the 13 μm feature. A study of ISO-SWS spectra of oxygen-rich AGB stars. Astron. Astrophys., 352, pp. 609–618.

    ADS  Google Scholar 

  • Prinn, R G. 1993. Chemistry and evolution of gaseous circumstellar disks. In Protostars & Planets III, eds. E. H. Levy and J. I. Lunine (Tucson: Univ. Arizona Press), pp. 1005–1028.

    Google Scholar 

  • Puget, L. J., and Leger, A. 1989. A new component of the interstellar matter: small grains and large aromatic molecules. Ann. Rev. Astron. Astrophys., 27, pp. 161–198.

    ADS  Google Scholar 

  • Roques, F., Scholl, H., Sicardy, B., and Smith, B. A. 1994. Is there a planet around β Pictoris? Perturbations of a planet on a circumstellar dust disk. I. The numerical model. Icarus, 108, pp. 37–58.

    ADS  Google Scholar 

  • Rowan-Robinson, M. 1992. Interstellar dust in galaxies. Mon. Not. Roy. Astron. Soc., 258, pp. 787–799.

    ADS  Google Scholar 

  • Sandford, S. A., Allamandola, L. J., Tielens, A. G. G. M., and Valero, G. J. 1988. Laboratory studies of the infrared spectral properties of of CO in astrophysical ices. Astrophys. J., 329, pp. 498–510.

    ADS  Google Scholar 

  • Sandford, S. A., Pendleton, Y. J., and Allamandola, L. J. 1995. The galactic distribution of aliphatic hydrocarbons in the diffuse interstellar medium. Astmphys. J., 440, pp. 697–705.

    ADS  Google Scholar 

  • Schalén, C. 1929. Zur Frage der allgemeinen Absorption des Lichtes im Weltraum. Astmn. Nachr., 236, pp. 249–258.

    ADS  MATH  Google Scholar 

  • Schalén, C. 1934. Untersuchungen liber Dunkelnebel. Medd. Astmn. Obs. Upsala, No. 58.

    Google Scholar 

  • Schnaiter, M., Mutschke, H., Henning, Th., Lindackers, D., Strecker, M., and Roth, P. 1996. Ultraviolet spectroscopy of matrix-isolated amorphous carbon particles. Astmphys. J., 464, pp. L187–L190.

    ADS  Google Scholar 

  • Schnaiter, M., Mutschke, H., Dorschner, J., Henning, Th., and Salama, F. 1998. Matrixisolated nano-sized carbon grains as an analog for the 217.5 nanometer feature carrier. Astmphys. J., 498, pp. 486–496.

    ADS  Google Scholar 

  • Schoenberg, E., and Jung, B. 1934. Uber die Lichtstreuung im interstellaren Raum durch Wolken metallischere Partikel. Astron. Nachr.., 253, pp. 261–272.

    ADS  Google Scholar 

  • Schutte, W. A. 1996. Formation and evolution of interstellar icy grain mantles. In The Cosmic Dust Connection, ed. J. M. Greenberg (Dordrecht: Kluwer Academ. Publ.), NATO ASI Ser. C, Vol. 487, pp. 1–42.

    Google Scholar 

  • Schutte, W. A. 1999. Ices in the interstellar medium. In Laboratory Astmphysics and Space Research, eds. P. Ehrenfreund, C. Kraft, H. Kochan, and V. Pirronello (Dordrecht: Kluwer), pp. 69–103.

    Google Scholar 

  • Schutte, W. A., Tielens, A. G. G. M., Whittet, D. C. D., + 6 authors 1996. The 6.0 and 6.8 μm absorption features in the spectrum of NGC 7538: IRS9. Astron. Astmphys., 315, pp. L333–L336.

    Google Scholar 

  • Schutte, W. A., van der Hucht, K. A., Whittet, D. C. B., + 8 authors 1998. ISO-SWS observations of infrared absorption bands of the diffuse interstellar medium: The 6.2 μm feature of aromatic compounds. Astmn. Astmphys., 337, pp. 261–274.

    ADS  Google Scholar 

  • Seahra, S. S., and Duley, W. W. 1999. Extended Red Emission from carbon clusters in interstellar clouds. Astmphys. J., 520, pp. 719–723.

    ADS  Google Scholar 

  • Sedlmayr, E. 1994. From molecules to grains. In Molecules in the Stellar Envimnment, ed. U. G. JØrgensen (Berlin: Springer-Verlag), pp. 163–185.

    Google Scholar 

  • Sellgren, K. 1989. Infrared emission from reflection nebulae. In Interstellar Dust: Pmc. IAU Symp., bf 135, eds. L. J. Allamandola and A. G. G. M. Tielens (Dordrecht: Kluwer Academ. Publ.), pp. 103–108.

    Google Scholar 

  • Sellgren, K. 1994. Tiny grains, large molecules, and the infrared cirrus. In The First Symposium on the Infrared Cirrus and Diffuse Interstellar Clouds, eds. R. Cutri and W. B. Latter (San Francisco: Astron. Soc. Pacific), A. S. P. Conf. Ser., Vol. 58, pp. 243–254.

    Google Scholar 

  • Sellgren, K., Smith, R. G., Brooke, T. Y. 1994. The 3.2-3.6 micron spectra of Monoceros R2/IRS-3 and Elias 16. Astmphys. J., 433, pp. 179–186.

    ADS  Google Scholar 

  • Sellgren, K., Brooke, T. Y., Smith, R. G., Geballe, T. R. 1995. A new 3.25 micron absorption feature toward Monoceros R2/IRS3. Astmphys. J., 449, pp. L69–L72.

    ADS  Google Scholar 

  • Serkowski, K. 1973. Interstellar polarization. In Interstellar Dust and Related Topics: Pmc. IAU Symp. 52, eds. J. M. Greenberg and H. C. van de Hulst (Dordrecht: Reidel), pp. 145–152.

    Google Scholar 

  • Siebenmorgen, R., and Krligel, E. 1992. Dust model containing polycyclic aromatic hydrocarbons in various environments. Astmn. Astmphys., 259, pp. 614–626.

    ADS  Google Scholar 

  • Sitko, M. L., Halbedel, E. M., Lawrence, G. F., Smith, J. A., and Yanow, K. 1994. Variable extinction in the HD 45677 and the evolution of dust grains in pre-main-sequence disks. Astmphys. J., 432, pp. 753–762.

    ADS  Google Scholar 

  • Skinner, C. J., and Whitmore, B. 1988. Circumstellar environments - IV. Mass-loss rates for carbon stars. Mon. Not. Roy. Astmn. Soc., 234, pp. 79p–84p.

    ADS  Google Scholar 

  • Sloan, G. C., and Price, S. D. 1995. Silicate emission at 10 microns in variables on the asymptotic giant branch. Astmphys. J., 451, pp. 758–767.

    ADS  Google Scholar 

  • Sloan, G. C., and Price, S. D. 1998. The infrared spectral classification of oxygen-rich dust shells. Astmphys. J. Suppl. Ser., 119, pp. 141–158.

    ADS  Google Scholar 

  • Smith, B. 1994. 10 years of Beta Pictoris - a personal reminiscence. In Circumstellar Dust Disks and Planet Formation, eds. R. Ferlet and A. Vidal-Madjar (Gif sur Yvette: Editions Frontières), pp. 1–3.

    Google Scholar 

  • Smith, R. G., Sellgren, K., and Brooke, T. Y. 1993. Grain mantles in the Taurus dark cloud. Mon. Not. Roy. Astron. Soc., 263, pp. 749–766.

    ADS  Google Scholar 

  • Sodroski, T. J., Dwek, E., Hauser, M. G., and Kerr, F. J. 1989. Dust energetics in the gas phases of the interstellar medium: The origin of the galactic large-scale far-infrared emission observed by IRAS. Astrophys. J., 336, pp. 762–779.

    ADS  Google Scholar 

  • Sodroski, T. J., Bennett, C., Boggess, N., + 8 authors 1994. Large-scale characteristics of interstellar dust from COBE DIRBE observations. Astrophys. J., 428, pp. 638–646.

    Google Scholar 

  • Sofia, U. J., Cardelli, J. A., and Savage, B. D. 1994. The abundant elements in the interstellar dust. Astrophys. J., 430, pp. 650–666.

    ADS  Google Scholar 

  • Sorrell, W. F. 1990. The ⋋ 2175-Å feature from irradiated graphite particles. Mon. Not. Roy. Astron. Soc., 243, pp. 570–587.

    ADS  Google Scholar 

  • Spaans, M., and Ehrenfreund, P. 1999. The interstellar medium: a general introduction. In Laboratory Astrophysics and Space Research, eds. P. Ehrenfreund, C. Kraft, H. Kochan, and V. Pirronello (Dordrecht: Kluwer), pp. 1–36.

    Google Scholar 

  • Speck, A. K., Barlow, M. J., and Skinner, C. J. 1997. The nature of silicon carbide in star outflows. Monthly Not. R. Astron. Soc., 288, pp. 431–456.

    ADS  Google Scholar 

  • Speck, A. K., Barlow, M. J., Sylvester, R. J. and Hofmeister, A. M. 2000. Dust features in the infrared spectra of oxygen-rich evolved stars. Astron. Astrophys. Suppl. Ser., 146, pp. 437–467.

    ADS  Google Scholar 

  • Stebbins, J., and Whitford, A. E. 1943. Six-color photometry of stars. I. The law of space reddening from the colors of 0 and B stars. Astrophys. J., 98, pp. 20–32.

    ADS  Google Scholar 

  • Stecher, T. P. 1965. Interstellar extinction in the ultraviolet. Astrophys. J., 142, pp. 1683–1684.

    ADS  Google Scholar 

  • Stein, W. A., and Gillett, F. C. 1969. Spectral distribution of infrared radiation from the Trapezium region of the Orion Nebula. Astrophys. J., 155, pp. L197–L199.

    ADS  Google Scholar 

  • Sterzik, M. F., and Morfill, G. E. 1994. Evolution of protoplanetary disks with condensation and coagulation. Icarus, 111, pp. 536–546.

    ADS  Google Scholar 

  • Sylvester, R. J., Barlow, M. J., Skinner, C. J., and Mannings, V. 1996. Optical, infrared, and millimetre-wave properties of Vega-Like systems Mon. Not. R. Astron. Soc., 279, pp. 925–939.

    Google Scholar 

  • Tanaka, M., Sato, S., Nagata, T., and Yamamoto, T. 1990. Three micron ice-band features in the p Ophiuchi sources Astrophys. J., 352, pp. 724–730.

    Google Scholar 

  • Taylor, A., Baggaley, W. J., and Steel, D. J. 1996. Discovery of interstellar dust entering the earth’s atmosphere. Nature, 380, pp. 323–325.

    ADS  Google Scholar 

  • Telesco, C. M., and Knacke, R. F. 1991. Detection of silicates in the beta Pictoris disk. Astrophys. J. Lett., 372, pp. L29–L31.

    ADS  Google Scholar 

  • Teixeira, T. C., Devlin, J. P., Buch, V., and Emerson, J. P. 1999. Discovery of solid HDO in grain mantles. Astron. Astrophys., 347, pp. L19–L22.

    ADS  Google Scholar 

  • Tielens, A. G. G. M. 1990. Carbon stardust: From soot to diamonds. In Carbon in the Galaxy: Studies from Earth and Space., eds. J. C. Tarter, S. Chang, and D. J. DeFrees (Washington: NASA), CP-3061, pp. 59–111.

    Google Scholar 

  • Tielens, A. G. G. M. 1995. The interstellar medium. In Airborne Astronomy Symposium on the Galactic Ecosystem: from Gas to Stars to Dust, ed. M. R. Haas, J. A. Davidson, E. F. Erickson (San Francisco: Astron. Soc. Pacific), A. S. P. Conf. Ser., Vol. 73, pp. 3–2l.

    Google Scholar 

  • Tielens, A. G. G. M., Tokunaga, A. T., Geballe, T. R., and Baas, F. 1991. Interstellar solid CO: polar and nonpolar interstellar ices. Astrophys. J., 381, pp. 181–199.

    ADS  Google Scholar 

  • Tielens, A. G. G. M., Wooden, D. H., Allamandola, L. J., Bregman, J., and Witteborn, F.C. 1996. The infrared spectrum of the Galactic Center and the composition of interstellar dust. Astrophys. J., 461, pp. 210–222.

    ADS  Google Scholar 

  • Treffers, R., and Cohen, M. 1974. High-resolution spectra of cool stars in the 10- and 20- micron region. Astrophys. J., 188, pp. 545–552.

    ADS  Google Scholar 

  • Triimpler, R. 1930. Preliminary results on the distances, dimensions, and space distribution of open star clusters. Lick Obs. Bull., No. 420.

    Google Scholar 

  • Van de Hulst, H. C. 1949. The solid particles in interstellar space. Rech. Astron. Obs. Utrecht, 11, pt. 2.

    Google Scholar 

  • Van Dishoeck, E. 1999. Models dnd observations of gas-grain interactions chemical evolution in star-forming regions. In Formation and Evolution of Solids in Space, ed. J. M. Greenberg, A. Li (Dordrecht: Kluwer Academ. Publ.), NATO ASI Ser. C, Vol. 523, pp. 229–264.

    Google Scholar 

  • Verschuur, G. L. 1989. Interstellar Matters. Essays on Curiosity and Astronomical Discovery (New York: Springer-Verlag).

    Google Scholar 

  • Vrba, F. J., Coyne, G. V., and Tapia, S. 1981. Observations of grain and magnetic field properties of the R Coronae Australis dark cloud. Astrophys. J., 243, pp. 489–511.

    ADS  Google Scholar 

  • Vrba, F. J., Coyne, G. V., and Tapia, S. 1993. An investigation of grain properties in the p Ophiuchi dark cloud. Astron. J., 105, pp. 1010–1026.

    ADS  Google Scholar 

  • Volk, K., Kwok, S., and Hrivnak, B. J. 1999. High-rsolution Infrared Space Observatory Spectroscopy of the unidentified 21 micron feature. Astrophys. J., 516, pp. L99–L102.

    ADS  Google Scholar 

  • Walmsley, C. M., and Schilke, P. 1993. Observations of hot molecular cores. In Dust and Chemistry in Astronomy, eds. T. J. Millar, and D. A. Williams (Bristol: Inst. Physics Publ.), pp. 37–52.

    Google Scholar 

  • Waters, L. B. F. M., Molster, F. J., de Jong, T., + 34 authors 1996. Mineralogy of oxygen-rich dust shells. Astron. Astrophys., 315, pp. L361–L364.

    Google Scholar 

  • Waters, L. B. F. M., Cami, J., De Jong, T., Molster, F. J., Van Loon, J. Th., Bouwman, J., De Koter, A., Waelkens, C., Van Winckel, H., and Morris, P. W. 1998a. An oxygen-rich dust disk surrounding an evolved star in the Red Rectangle. Nature, 391, pp. 868-....

    ADS  Google Scholar 

  • Waters, L. B. F. M., Beintema, D. A., Zijlstra, A. A., De Koter, A., Molster, F. J., Bouwman, J., De Jong, T., Pottasch, S. R., and De Graauw, Th. 1998b. Crystalline silicates in planetary nebulae with [WC] central stars. Astron. Astrophys., 331, pp. L61–L64.

    ADS  Google Scholar 

  • Webster, A. 1995. The lowest of the strongly infrared active vibrations of the fullerenes and an astronomical emission band at a wavelength of 21 μm. Monthly Not. R. Astron. Soc., 277, pp. 1555–1566.

    ADS  Google Scholar 

  • Weintraub, D. A., and Stern, S. A. 1994. A reinterpretation of millimeter observations of nearby IRAS excess stars. Astron. J., 108, pp. 701–710.

    ADS  Google Scholar 

  • Whittet, D. C. B. 1984. Interstellar grain composition: a model based on elemental depletions. Mon. Not. Roy. Astron. Soc., 210, pp. 479–487.

    ADS  Google Scholar 

  • Whittet, D. C. B. 1992. Dust in the Galactic Environment, (Bristol: Inst. Physics Publ.).

    Google Scholar 

  • Whittet, D. C. B. 1993. Observations of molecular ices. In Dust and Chemistry in Astronomy, eds. T. J. Millar and D. A. Williams (Bristol: Inst. Physics Publ.), pp. 9–35.

    Google Scholar 

  • Whittet, D. C. B. 1996. Polarization of starlight by interstellar dust. In The Cosmic Dust Connection, ed. J. M. Greenberg (Dordrecht: Kluwer Academ. Publ.), pp. 205–221.

    Google Scholar 

  • Whittet, D. C. B., Bode, M. F., Longmore, A. J., Adamson, A. J., McFadzean, A. D., Aitken, D. K., and Roche, P. F. 1988. Infrared spectroscopy of dust in the Taurus dark clouds: ice and silicate. Mon. Not. Roy. Astron. Soc., 233, pp. 321–326.

    ADS  Google Scholar 

  • Whittet, D. C. B., Martin, P. G., Hough, J. H., Rouse, M. F., Bailey, J. A., and Axon, D. J. 1992. Systematic variations in the wavelength dependence of interstellar linear polarization. Astrophys. J., 386, pp. 562–577.

    ADS  Google Scholar 

  • Whittet, D. C. B., Schutte, W. A., Tielens, A. G. G. M., Boogert, A. C. A., de Graauw, Th., Ehrenfreund, P., Gerakines, P. A., Helmich, F. P., Prusti, T., and van Dishoeck, E. F. 1996. An ISO SWS view of interstellar ices: first results. Astron. Astrophys., 315, pp. L357–360.

    ADS  Google Scholar 

  • Whittet, D. C. B., Boogert, A. C. A., Gerakines, P. A. + 7 authors 1997. Infrared spectroscopy of dust in the diffuse interstellar medium toward Cygnus OB2 No.12. Astrophys. J., 490, pp. 729–734.

    ADS  Google Scholar 

  • Wildt, R. 1933. Kondensation in Sternatmospharen Zeitschr. f. Astrophys., 6, pp. 345–354.

    Google Scholar 

  • Williams, D. A. 1989. Grains in diffuse clouds: carbon-coated silicate cores. In Interstellar Dust: Proc. IAU Symp., 135, eds. L. J. Allamandola and A. G. G. M. Tielens (Dordrecht: Kluwer Academ. Publ.), pp. 367–373.

    Google Scholar 

  • Witt, A. N. 1989. Visible/UV scattering by interstellar dust. In Interstellar Dust: Proc. IAU Symp., 135, eds. L. J. Allamandola and A. G. G. M. Tielens (Dordrecht: Kluwer Academ. Publ.), pp. 87–100.

    Google Scholar 

  • Witt, A. N., Petersohn, J. K., Bohlin, R. C., O-Connell, R. W., Roberts, M. S., Smith, A. M., and Stecher, T. P. 1992. Ultraviolet Imaging Telescope images of the reflection nebula NGC 7023: Derivation of ultraviolet scattering properties of dust grains. Astrophys. J. Lett., 395, pp. L5–L8.

    ADS  Google Scholar 

  • Witt, A. N., Gordon, K. D., Furton, D. G. 1998. Silicon nanoparticles: source of extended red emission? Astrophys. J., 501, pp. L111–L114.

    ADS  Google Scholar 

  • Wolff, M. J., Clayton, G. C., Kim, S.-H., Martin, P. G. 1997. Ultraviolet interstellar linear polarization. III. Features. Astrophys. J., 478, pp. 395–402.

    ADS  Google Scholar 

  • Wright, E. L., Mather, J. C., Bennett, C. L., + 19 authors 1991. Preliminary spectral observations of the Galaxy with a 7° beam by the Cosmic Background Explorer (COBE). Astrophys. J., 381, pp. 200–209.

    ADS  Google Scholar 

  • Wurm, G., Blum, J. 1998. Experiments on preplanetary dust aggregation. Icarus, 132, pp. 125–136.

    ADS  Google Scholar 

  • Yamashita, T., Handa, T., Omodaka, T., Kitamura, Y., Kawazoe, E., Hayashi, S. S., and Kaifu, N. 1993. Upper limits to the CO J = 1--0 emission around Vega-Like stars: gas depletion of the circumstellar ring around ε Eridani. Astrophys. J. Lett., 402, pp. L65–L67.

    ADS  Google Scholar 

  • Zinner, E. 1997. Presolar material in meteorites: an overview. In Astrophysical Implications of the Laboratory Study of Presolar Material, eds. T. J. Bernatowicz and E. Zinner, AIP Conf. Ser. Proceed., 402, pp. 3–26.

    Google Scholar 

  • Zinner, E., Amari, S., Wopenka, B., and Lewis, R. S. 1995. Interstellar graphite in meteorites: Isotopic compositions and structural properties of single graphite grains from Murchison. Meteoritics, 30, pp. 209–226.

    ADS  Google Scholar 

  • Zubko, V. G., Smith, T. L., and Witt, A. N. 1999. Silicon nanoparticles and interstellar extinction. Astrophys. J., 511, pp. L57–L60.

    ADS  Google Scholar 

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  1. SchillergiiBchen 3, Astrophysikalisches Institut, 07745, Jena, Germany

    Johann Dorschner

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    Bo Å. S. Gustafson  & Stan Dermott  & 

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Dorschner, J. (2001). Interstellar Dust and Circumstellar Dust Disks. In: Grün, E., Gustafson, B.Å.S., Dermott, S., Fechtig, H. (eds) Interplanetary Dust. Astronomy and Astrophysics Library. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-56428-4_14

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