Abstract
Studies of the ultraviolet spectra of hot interacting binaries reveal methods that may represent important new tools for probing the physical conditions in the winds emanating from hot stars. Two systems, Mu Sagittarii and UW CMa are taken as examples of how these methods can be utilized to investigate the physics of mass loss in such objects.
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© 1988 Kluwer Academic Publishers
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Bruhweiler, F.C. (1988). Interacting Binaries and Mass Loss in Hot Stars. In: Bianchi, L., Gilmozzi, R. (eds) Mass Outflows from Stars and Galactic Nuclei. Astrophysics and Space Science Library, vol 142. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2941-8_7
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DOI: https://doi.org/10.1007/978-94-009-2941-8_7
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