SKYLAB ultraviolet stellar spectra - Cool stars with hot secondaries

Details SKYLAB ultraviolet stellar spectra - Cool stars with hot secondaries SKYLAB ultraviolet stellar spectra - Cool stars with hot secondaries

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...203..435p&link_type=abstract

Astrophysical Journal, vol. 203, Jan. 15, 1976, pt. 1, p. 435-437.

Astronomy and Astrophysics

Astrophysics

18

Astronomical Catalogs, Binary Stars, Cool Stars, Stellar Spectra, Ultraviolet Spectroscopy, Giant Stars, Skylab Program, Stellar Luminosity, Subdwarf Stars, Supergiant Stars, Ultraviolet Spectrometers

Scientific paper

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.

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