Skylab ultraviolet stellar spectra: Cool stars with hot secondaries
Journal Article
·
· Astrophys. J.; (United States)
A hot companion to the G5 III star HR 3080, a single-line spectroscopic binary, has been discovered from spectra in the vacuum-ultraviolet. The companion must be a subdwarf or pre-white dwarf. A list of previously known systems of the zeta Aur and VV Cep type observed with the ultraviolet spectrograph on Skylab is also given. (AIP)
- Research Organization:
- Department of Astronomy, University of Texas at Austin
- OSTI ID:
- 7285866
- Journal Information:
- Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 203:2; ISSN ASJOA
- Country of Publication:
- United States
- Language:
- English
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