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Limits on diffuse X-ray emission from M101Observed limits on diffuse X-ray emission from M101 require that the temperature of any coronal or matrix hot gas which is radiating an appreciable part (10 percent) of the average supernova power be less than 10(5.7)K. Furthermore, the fraction of the galactic plane occupied by hot bubbles similar to the one which apparently surrounds the sun is at most 25 percent in the region between 10 kpc and 20 kpc from the galactic center.
Document ID
19850041266
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/162674
Authors
Mccammon, D. (Wisconsin Univ. Madison, WI, United States)
Sanders, W. T. (Wisconsin, University Madison, WI, United States)
Date Acquired
August 12, 2013
Publication Date
December 1, 1984
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 287
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
85A23417
Funding Number(s)
CONTRACT_GRANT: NAG8-431
Distribution Limits
Public
Copyright
Other

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