Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...266..755m&link_type=abstract
Astrophysical Journal, Part 1, vol. 266, Mar. 15, 1983, p. 755-760.
Astronomy and Astrophysics
Astronomy
11
Eclipsing Binary Stars, Iue, Peculiar Stars, Stellar Spectrophotometry, Ultraviolet Spectroscopy, Variable Stars, Far Ultraviolet Radiation, Photosphere, Radial Velocity, Satellite Observation, Spaceborne Astronomy, Stellar Evolution
Scientific paper
The eclipsing binary system R Arae = HD 149730 is a relatively bright southern system with an orbital period of about 4.4 days. It is a single-lined spectroscopic binary. The spectral class of the primary component is B9 Vp. The system was included in a study of mass flow and evolution in close binary systems using the International Ultraviolet Explorer satellite (IUE). Four spectra in the wavelength range from 1150 to 1900 A were obtained with the far-ultraviolet SWP camera, and six spectra in the range from 1900 to 3200 range were obtained with the mid-ultraviolet LWR camera. The close binary R Arae exhibits very unusual ultraviolet spectra. It appears that no other close binary system, observed with any of the orbiting satellites, shows outside-eclipse ultraviolet continuum flux variations of this nature.
Kondo Yoshihiko
McCluskey George E.
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