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VV Puppis - The soft X-ray machineThe detection of soft and hard X rays from VV Pup is reported, and an orbital light curve is presented for both. The light curves are found to be in good agreement with the orbital light curve observed in the optical (Warner and Nather, 1972), suggesting that both X rays and optical light arise from the vicinity of a bright spot near one magnetic pole of the white dwarf. The radius of the soft X-ray-emitting bright spot is in the range 20-120 km, and its temperature is in the range (2-6) x 10 to the 5th K. The observed ratio of soft X-ray to hard X-ray fluxes is approximately 15, the highest of all the AM Her stars.
Document ID
19840050800
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Patterson, J.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Lamb, D. Q.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Fabbiano, G.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Raymond, J. C.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Beuermann, K.
(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; Max-Planck-Institut fuer Physik und Astrophysik Garching, Germany)
Swank, J.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
White, N. E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 12, 2013
Publication Date
April 15, 1984
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 279
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
84A33587
Funding Number(s)
CONTRACT_GRANT: NAG5-87
CONTRACT_GRANT: NAGW-246
Distribution Limits
Public
Copyright
Other

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