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Rocket observations of the Perseus X-ray sourceThe spectrum and angular distribution of soft X-ray emission from the source in the Perseus cluster has been observed. A prominent feature of this source is a point-like component at the position of NGC 1275. Preliminary analysis indicates that the spectrum of this source does not rise as steeply at energies below 1 keV as has been reported previously.
Document ID
19750051493
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Catura, R. C.
Acton, L. W. (Lockheed Research Laboratories Palo Alto, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1975
Subject Category
Astronomy
Meeting Information
Meeting: International Conference on X-Rays in Space - Cosmic, Solar, and Auroral X-Rays, Calgary
Location: Alberta
Country: Canada
Start Date: August 14, 1974
End Date: August 21, 1974
Accession Number
75A35565
Funding Number(s)
CONTRACT_GRANT: NASW-2672
CONTRACT_GRANT: NASW-2414
Distribution Limits
Public
Copyright
Other

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