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X-ray emission from Be star binariesA model in which a neutron star in an eccentric inclined orbit around a Be star passes through a ring of matter around the Be star has been used to explain the recurrent flares of X-ray emission from these systems. The optical emission during X-ray flares is due to partial absorption and reprocessing of the X-rays in the ring.
Document ID
19850053279
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/163155
Authors
Apparao, K. M. V. (NASA Marshall Space Flight Center Space Science Laboratory, Huntsville, AL; Tata Institute of Fundamental Research, Bombay, India)
Date Acquired
August 12, 2013
Publication Date
May 1, 1985
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 292
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
85A35430
Distribution Limits
Public
Copyright
Other

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