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Ultraviolet spectroscopy of binary systemsFour typical binary systems that illustrate some of the major problems in the study of binary stars are discussed. Consideration is given to (1) high-luminosity X-ray sources typified by Cyg X-1 (HDE 226868) and Vela XR-1 (HD 77581), (2) low-luminosity X-ray sources (HZ Her), (3) late-type systems of W UMa and RS CVn type, and (4) cool supergiants with a hot companion (VV Cephei).
Document ID
19800069577
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Dupree, A. K. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Hartmann, L. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Raymond, J. C. (Harvard-Smithsonian Center for Astrophysics Cambridge, Mass., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1980
Subject Category
Astronomy
Meeting Information
Meeting: Close binary stars: Observations and interpretation
Location: Toronto
Country: Canada
Start Date: August 7, 1979
End Date: August 10, 1979
Accession Number
80A53747
Funding Number(s)
CONTRACT_GRANT: NSG-7176
CONTRACT_GRANT: NSG-5370
Distribution Limits
Public
Copyright
Other

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