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Binary modulation and transient periodic variations in X-ray emission from the AM Her binary H 0139 - 68A detailed timing analysis of HEAO-1 and Einstein satellite soft X-ray data on the AM Her-type binary H 0139 - 68 indicates that the X-ray flux is modulated at the 113.6363-min period of its optical counterpart, and that the X-ray source shows high and low states. Transient X-ray pulsations with a period of about 275 sec are noted in the Imaging Proportional Counter (IPC) data during the high state, and the rapid X-ray flickering observed in the IPC light curve is characterized by an average e-folding autocorrelation time of about 10-20 sec. The present optical and X-ray data preclude the presence of an accretion disk in the primary system.
Document ID
19840053240
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Singh, K. P.
(Tata Inst. of Fundamental Research Bombay, India)
Agrawal, P. C.
(Tata Institute of Fundamental Research Bombay, India)
Riegler, G. R.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Date Acquired
August 12, 2013
Publication Date
June 1, 1984
Publication Information
Publication: Royal Astronomical Society, Monthly Notices
Volume: 208
ISSN: 0035-8711
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0035-8711
Accession Number
84A36027
Distribution Limits
Public
Copyright
Other

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