An empirical comparison of X-ray and radio emission from supernova remnants

Details An empirical comparison of X-ray and radio emission from supernova remnants An empirical comparison of X-ray and radio emission from supernova remnants

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...205..238s&link_type=abstract

Astrophysical Journal, vol. 205, Apr. 1, 1976, pt. 1, p. 238-246. ERDA-sponsored research.

Computer Science

Sound

10

Astronomical Catalogs, Radio Emission, Supernova Remnants, X Ray Sources, Luminosity, Radio Sources (Astronomy), Rocket Sounding, Statistical Correlation

Scientific paper

Data from several rocket flights are combined to list upper limits to soft X-ray emission from supernova remnants (SNRs). These limits are compared with observations of SNRs that are known X-ray emitters. There is no strong correlation between measured radio and X-ray flux at the top of the atmosphere. X-ray luminosities and upper limits are calculated for all SNR that are bright radio sources. The ratio between X-ray and radio luminosity is found to be in the range from 20 to 2000. The dependence of SNR luminosity on diameter is discussed.

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