Abstract
Dust can be included in the photoionization models of planetary nebulae; the dust temperatures resulting from the radiation field within the models can be evaluated and the resulting thermal IR emission compared to observations. We use a model of NGC 3918 to illustrate the behavior of various grain materials (graphite, amorphous carbon, silicates, and iron). We also present a model of IC 418 with graphite grains in both the ionized zone and in a surrounding thick, neutral shell.
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References
Adams, S. 1983. Ph. D. Thesis, University College London.
Borghesi, A., Bussoletti, E., and Colangeli, L. 1985. Astron. Astrophys., 142, 225.
Clegg, R.E.S., Harrington, J.P., and Barlow, M.J. 1984. ‘Proc. European IUE Conference’, ESA SP-218, p. 337.
Clegg, R.E.S., Harrington, J.P., Barlow, M.J., and Walsh, J.R. Astrophys. J., (March 1987).
Cohen, M., and Barlow, M.J. 1980. Astrophys. J., 238, 585.
Cohen, M., Harrington, J.P., and Hess, R. 1984. Astrophys. J., 283, 687.
Draine, B.T. 1985. Astrophys. J. Suppl., 52, 587.
Draine, B.T., and Lee, H.M. 1984. Astrophys. J., 285, 89.
Forrest, W.J., Houck, J.R., and McCarthy, J.F. 1981. Astrophys. J., 248, 195.
Goebel, J.H., and Moseley, S., 1985. Astrophys.J.,290, L35.
Harrington, J.P., Monk, D.J., and Clegg, R.E.S. 1987. To be submitted.
kunasz, P.B., Hummer, D.G., and Mihalas, D. 1975. Astrophys. J., 202. 92.
Lenham, A.P. and Treherne, D.M. 1966. In ‘Optical Properties and Electronic Structure of Metals and Alloys’, ed. Abeles, F., ( Amsterdam: North-Holland Pub. Co. ) p. 196.
Leroy, J.L., Le Borgne, J.F., Arnaud, J. 1986. Astron. Astrophys., 160, 171.
Mathis, J.S., Rumpl, W., and Nordsiek, K.H. 1977. Astrophys. J., 217, 425.
Moravec, T.J., Rife, J.C., and Dexter, R.N. 1976. Phys. Rev. B, 13, 3297.
Moseley, H. 1980. Astrophys. J., 238, 892.
Natta, A., and Panagia, N. 1976. Astron. Astrophys., 50, 211.
Natta, A., and Panagia, N. 1981. Astrophys. J., 248, 189.
Pottasch, S.R., Baud, B., Beintema, D., Emerson, J., Habing, H.J., Jennings, R., and Marsden, P. 1984. Astron. Astrophys., 138, 10.
Pottasch, S.R., Preite-Martinez, A., Olnon, F.M., Mo Jing-Er, and Kingma, S. 1986. Astron. Astrophys., 161, 363.
Reay, N.K., and Worswick, S.P. 1979. Astron. Astrophys., 72, 31.
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© 1987 D. Reidel Publishing Company
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Harrington, J.P. (1987). Modeling the Thermal Emission From Dust in Planetary Nebulae. In: Planetary and Proto-Planetary Nebulae: From IRAS to ISO. Astrophysics and Space Science Library, vol 135. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3891-5_27
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DOI: https://doi.org/10.1007/978-94-009-3891-5_27
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