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Skylab ultraviolet stellar spectra: Cool stars with hot secondaries

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/154094· OSTI ID:7285866
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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