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Recent Spectroscopy of X-Ray Sources and Systems Related to Cataclysmic Variables: II
Published online by Cambridge University Press: 12 April 2016
Abstract
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Spectroscopic observations of two very different objects are discussed: the first, SS433, is a wery massive binary system probably containing an unseen 0 or WR star and a black hole surrounded by a luminous precessing accretion disk (from which emanate spectacular relativistic jets); the second, GK Per, is a classical old nova consisting of a slightly evolved K2 star and an unseen white dwarf companion surrounded by an accretion disk which is less luminous than the K2 star.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 72: Cataclysmic Variables and Related Objects , 1983 , pp. 25 - 28
- Copyright
- Copyright © Reidel 1983
References
REFERENCES
Crampton, D., Cowley, A.P., and Hutchings, J.B.
1980, Ap.J.(Letters), 235, L131 (CCH).Google Scholar
Kemp, J.C., Barhous, M.S., Kemp, G.N., and Hagood, D.M.
1981, Proc. of Rome Meeting on SS433, Vistas in Astronomy, 25, 31.Google Scholar
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