Variable, optically thick, hot plasma observed in interacting binaries

Details Variable, optically thick, hot plasma observed in interacting binaries Variable, optically thick, hot plasma observed in interacting binaries

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..99..281k&link_type=abstract

(International Astronomical Union, Colloquium on Double Stars, Physical Properties and Generic Relations, 80th, Bandung, Indones

Astronomy and Astrophysics

Astrophysics

9

Binary Stars, Space Plasmas, Stellar Envelopes, Ultraviolet Spectra, Variable Stars, High Temperature Plasmas, Iue, Light Curve, Optical Thickness, Spectral Energy Distribution, Stellar Evolution

Scientific paper

Recent International Ultraviolet Explorer (IUE) observations of two interacting binaries, R Arae and HD 207739 are reported. The ultraviolet spectra indicate the presence of optically-thick, variable hot plasma in those binary systems. These two binaries may belong to a class of binaries that are currently undergoing a rarely observed and probably short-lived phase in their evolution. Their properties are compared with those of two other interacting binaries, U Cephei and Beta Lyrae.

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