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The hot components of hydrogen deficient binariesLow resolution IUE observations of the hot components of three very similar but peculiar objects: LSS 4300, Upsilon Sgr, and KS Per were compared. The possible evolutionary scenarios from observations and the extremely low hydrogen contents of the visible stars are discussed. It is suggested that the hot secondaries in hydrogen deficient binaries should also be hydrogen deficient.
Document ID
19820023383
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Drilling, J. S. (Louisiana State Univ. Baton Rouge, LA, United States)
Schoenberner, D. (Louisiana State Univ. Baton Rouge, LA, 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
82N31259
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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