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Upper limits on the cyclotron lines from Her X-1 as observed with OSO-8Observations of Her X-1 were obtained during its ON-state in September, 1977, with the high-energy X-ray detector on board OSO-8. Upper limits on the line fluxes at 60 and 135 keV based on these observations are above, and hence consistent with, the positive results reported by Trumper, et al from a balloon flight during the same time interval. A detailed analysis of the time-variable et al background spectrum suggests that the line emission, especially in the time-averaged spectrum of Her X-1 previously reported by other workers at 25, 60, and 135 keV, is due to instrumental effects. The spectrum obtained with OSO-8 in September, 1977, is considerably steeper than that observed in pre-1976 balloon flights. These results are consistent with the results obtained by Trumper showing a decrease in the effective temperature of Her X-1 between May, 1976, and September, 1977.
Document ID
19780024050
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Dennis, B. R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Maurer, G. S.
(Catholic Univ. of Am. Washington, D. C., United States)
Cutler, E. P.
(Comtech Lanham, Md., United States)
Crannell, C. J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Dolan, J. F.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Frost, K. J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Orwig, L. E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 9, 2013
Publication Date
August 1, 1978
Publication Information
Publication: ma Ray Spectry. In Astrophys.
Subject Category
Space Radiation
Accession Number
78N31993
Funding Number(s)
CONTRACT_GRANT: NSG-5066
CONTRACT_GRANT: NAS5-24451
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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