Abstract
The International Ultraviolet Explorer is one of the most successful astronomical satellites. It has been operating now since more than 10 years. IUE was launched on 26th January 1978. The satellite consists of a spacecraft of 312 kg with 122 kg of instruments. It is an elliptical orbit with an altitude varying between 26000 and 46000 km. The telescope, a 45 cm Cassegrain has a 16 arc.min field of view. There are two spectrographs: a short wavelength spectrograph, operating between 1150 and 1950 Å with a high solution mode of 0.15 Å resolution, and a low resolution mode of 6 Å resolution. The long wavelength spectrograph operates between 1900 Å and 3200 Å, with a high resolution mode of 0.25 Å, and a low resolution mode of 7 Å. A detailed description of IUE, its history and its instruments can be found in “Exploring the Universe with IUE” (Kondo,1987).
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References
Exploring the Universe with the IUE Satellite, 1987, Y.Kondo (Reidel; Dordrecht).
Boggess, A. and Willson, R.: The History of IUE. p. 3.
Bohm-Vitense, E. and Querci, M.: Intrinsically Variable Stars, p. 223.
Cassinelli, J.P. and Lamers, H.J.G.L.M.: Winds from Young Hot Stars, p. 139.
Dupree, A.K. and Reimers, D.: Mass loss from Cool Stars, p. 321.
Jordan, C. and Linsky, J.L.: Chromospheres and Transition Regions, p. 259.
Snow, T.P. and Stalio, R.: Be-Star Phenomena, p. 183.
Vauclair, G. and Liebert, J.: The End Stages of Stellar Evolution: White Dwarfs. Hot Subdwarfs and Nuclei of Planetary Nebulae, p. 355.
Other References
Brugel, E.W., Beach, T.E., Wilson, L.A. and Bowen, G.H.: “1987 IAU Colloquia: The Symbiotic Phenomenon”.
Dupree, A.K. 1986, Ann. Rev. Astron. Astrophys., 24, 377.
Guinan, E.F. et al.: 1986 in “New Insights in Astrophysics: Eight Years of UV Astronomy With IUE”. ESA SP-263, p. 197.
Hartmann, L., Balinnas, L.S., Duncan, D.K. and Noyes, R.W.: 1984, Astrophys. J., 279, 778.
Henrichs, H.F., Hammerschlag-Hensberge, G., Howarth, I.D. and Barr, P.: 1983, Astrophys. J., 268, 807.
Kirschner, R.P.: 1988 in “A Decade of UV Astronomy With the IUE Satellite”. ESA SP-281, Vol. 1, p. 3.
Lamers, H.J.G.L.M.: 1987 in “Instabilities in Luminous Early Type Stars”, eds. Lamers and de Loore, (Reidel, Dordrecht), p. 99.
Mullan, D.J. and Stencel, R.E.: 1982, in “Advances in UV Astronomy: Four Years of IUE Research”, NASA CP-2238, p. 235.
Prinja, R.K., Howarth, I.D. and Henrichs, H.F.: 1987, Astrophys. J., 317, 389.
Rodono, M.: 1988, in “A Decade of UV Astronomy With the IUE Satellite”, ESA SP-281, Vol. 2, p. 45.
Sanz Ferandes de Cordoba, L. et al.: 1988, in “A Decade of UV Astronomy With the IUE Satellite”, ESA SP-281, Vol. 1, p. 115.
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© 1989 Springer-Verlag Berlin Heidelberg
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Lamers, H.J.G.L.M. (1989). A Decade of Stellar Research with IUE. In: Klare, G. (eds) Reviews in Modern Astronomy 2. Reviews in Modern Astronomy, vol 2. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-75183-7_3
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DOI: https://doi.org/10.1007/978-3-642-75183-7_3
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