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The nature of the X-ray nova A0620-00A model is presented for the X-ray nova A0620-00. Identification with a nova can be ruled out on two counts. A binary consisting of a late-type subgiant near the Roche lobe, irradiated by an accreting compact companion is shown, however, to be in agreement with all known observations. Photometry of the optical object should be pursued since variability on an approximately eight hour period is expected.
Document ID
19760018998
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Endal, A. S. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Devinney, E. J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Sofia, S. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1976
Publication Information
Publication: X-ray Binaries
Subject Category
Astronomy
Accession Number
76N26086
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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