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Soft X-ray results from the Wisconsin experiment on OSO-8Design features and capabilities of a soft X-ray instrument aboard OSO 8 are discussed, and results are presented for observations of AM Her, Her X-1, and Eta Car. The observations of AM Her indicate that: (1) the spectrum is composite, with a very steep or very-low-temperature component plus a rather flat or very-high-temperature component; (2) the relative phase of soft X-ray minimum and optical V-band primary minimum has remained stable over the interval between 1975 'high-state' observations and 1976 'low-state' observations; and (3) the times of soft X-ray minima and hard X-ray maxima coincide, to within the accuracy of the observations. For Her X-1, soft X-ray turn-on is found to lag behind hard X-ray turn-on by no more than 3 hr. It is suggested that little or no absorption of the soft X-ray component occurs during the on state by cool gas within the Her X-1 system. A strong source with a spectrum peaked between 0.4 and 1.5 keV has been detected which is consistent with a point source at the position of Eta Car.
Document ID
19780042068
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Bunner, A. N.
(Wisconsin, University Madison, Wis., United States)
Date Acquired
August 9, 2013
Publication Date
February 15, 1978
Publication Information
Publication: Astrophysical Journal
Subject Category
Astronomy
Accession Number
78A25977
Funding Number(s)
CONTRACT_GRANT: NAS5-22410
Distribution Limits
Public
Copyright
Other

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