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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%) of the average supernova power be less than 10(5.7)K. Furthermore, the fraction of the galactic plane occupied by hot buttles similar to the one which apparently surrounds the Sun is at most 25% in the region between 10 kpc and 20 kpc from the galactic center.
Document ID
19840010079
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Mccammon, D. (Wisconsin Univ. Madison, WI, United States)
Sanders, W. T. (Wisconsin Univ. Madison, WI, United States)
Date Acquired
September 4, 2013
Publication Date
January 1, 1984
Subject Category
Space Radiation
Report/Patent Number
NASA-CR-170978
NAS 1.26:170978
Accession Number
84N18147
Funding Number(s)
CONTRACT_GRANT: NAG8-431
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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