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continuum and emission lines in eta LyraeIntegral photometric characteristics of beta Lyrae were redetermined using its brightest visual companion, the star HD 174664. It was attempted to separate the fluxes coming from the two components. The flux distributions are badly contaminated by the radiation of the circumstellar hydrogen. Peculiarities seem to be present in both components; in particular, the secondary star cannot be represented by an atmosphere with a unique effective temperature, and best represented by a thick disk.
Document ID
19820023384
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Plavec, M. J. (University of Southern California Los Angeles, CA, United States)
Weiland, J. L. (University of Southern California Los Angeles, CA, United States)
Dobias, J. J. (University of Southern California Los Angeles, CA, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Publication Information
Publication: NASA. Goddard Space Flight Center Advan. in Ultraviolet Astron.
Subject Category
Astronomy
Accession Number
82N31260
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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