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An X-ray survey of nine historical novaeThe Einstein Observatory imaging proportional counter was used to search for X-ray emission from nine nearby historical novae. Six of the novae were detected with estimated X-ray intensities between .1 to 4 keV of 10 to the -13th power to 10 to the -11th power ergs/sq cm-s, comparable to the intensities of previously detected cataclysmic variables. The X-ray intensity of one of the novae, V603 Aql, varies over times of several hundred seconds. The data suggest a correlation between the decay rate of the historical outburst and the current X-ray luminosity. Alternatively, the X-ray luminosity may be related to the inclination of the binary system.
Document ID
19810004450
Acquisition Source
Legacy CDMS
Document Type
Preprint (Draft being sent to journal)
Authors
Becker, R. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Marshall, F. E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 4, 2013
Publication Date
September 1, 1980
Subject Category
Astrophysics
Report/Patent Number
NASA-TM-82014
Accession Number
81N12961
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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