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Optical study of the X-ray binary Hercules X-1The 1.7 day B-V light curve of HZ Herculis shows the existence of a small hot component which is present only during the X-ray active portion of the 35-day cycle. This hot component is associated with the X-ray source since it is absent during X-ray eclipse.
Document ID
19760059617
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Saint John, R. H. (New Mexico, University Albuquerque, N. Mex., United States)
Date Acquired
August 8, 2013
Publication Date
August 15, 1976
Publication Information
Publication: Astrophysical Journal
Volume: 208
Subject Category
Astrophysics
Accession Number
76A42583
Distribution Limits
Public
Copyright
Other

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