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A new AM Her-like X-ray sourceThe discovery of a new X ray source associated with a binary and classifiable as a member of the AM Her class of objects is reported. The object was located with a detector on the HEAO A-2 spacecraft and by the imaging proportional counter on the Einstein Observatory. Detection occurred in the 0.15-0.4 keV band, and intensity variations of a factor of 2 were observed to happen on a time scale of around 2 hr. A location error box 0.9 deg on a side was constructed from the 2.95 deg overlapping FWHM field of view of the HEAO detector. The object, designated HO139-68, was reexamined using photometric and spectroscopic scans of it and the companion, which has been observed to be an ordinary late type star. Evidence for the presence of a magnetic white dwarf in the binary is discussed, noting indications of cyclotron emission. The X ray source flux is estimated to be 2.3/10 billion erg per sq cm per sec.
Document ID
19830042050
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Agrawal, P. C.
(Tata Inst. of Fundamental Research Bombay, India)
Rao, A. R.
(Tata Institute of Fundamental Research Bombay, India)
Riegler, G. R.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Date Acquired
August 11, 2013
Publication Date
January 27, 1983
Publication Information
Publication: Nature
Volume: 301
Subject Category
Astronomy
Accession Number
83A23268
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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