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IUE Ultraviolet Spectra of V Sagittae

Published online by Cambridge University Press:  12 April 2016

Robert H. Koch ,
M. Javad Siah  and
Michael N. Fanelli
Robert H. Koch
Affiliation:
Department of Astronomy and Astrophysics, University of Pennsylvania
M. Javad Siah
Affiliation:
Department of Astronomy and Astrophysics, University of Pennsylvania
Michael N. Fanelli
Affiliation:
Department of Astronomy and Astrophysics, University of Pennsylvania

Extract

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V Sge is a short period, double-line spectroscopic and eclipsing close binary which is also intrinsically variable through a range of at most 3 mag in visual and photographic light. Almost all modern insight is founded upon the interpretation by Herbig, et al. (1965), who developed the evidence for the binary nature of the star, evaluated the nearly 0.5 day Keplerian period, studied the short-term Doppler and intensity variations of the spectrum, and obtained a limiting representation of the intrinsically noisy ultraviolet light curve. The orbital plane view of the binary, as developed by these authors, shows patchy distributions of 0 IIIf1 and 0 VI emissions and mass loss from the system as a whole.

Type
Colloquium Session VII
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 448 - 452
Copyright
Copyright © The University of Rochester 1979

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