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The 35-D X-ray profile of Her X-1Substantial X-ray emission as reported by Ariel 5 from Her X-l midway through the extended low-state portion of its 35-day cycle is examined. A similar feature during another cycle measured from UHURU satellite is also examined. It is proposed that this feature should occur regularly, consistent with some models for the mass accretion disc which have been reported in the literature. The results of the analysis of 500 days of Ariel-5 All-Sky Monitor data are reported which support the view that the feature occurs regularly in the 35-day cycle.
Document ID
19760024021
Acquisition Source
Legacy CDMS
Document Type
Preprint (Draft being sent to journal)
Authors
Holt, S. S.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Boldt, E. A.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Kaluzienski, L. J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Serlemitsos, P. J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Swank, J. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 3, 2013
Publication Date
August 1, 1976
Subject Category
Astronomy
Report/Patent Number
X-661-76-182
NASA-TM-X-71174
Accession Number
76N31109
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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