NASA NTRS · 19800069577
Ultraviolet spectroscopy of binary systems
Abstract
Four 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).
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Dupree, A. K., Hartmann, L., Raymond, J. C.. 1980-01-01. Ultraviolet spectroscopy of binary systems. https://ntrs.nasa.gov/citations/19800069577
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