The X-ray radiation of known-age supernova remnants

Details The X-ray radiation of known-age supernova remnants The X-ray radiation of known-age supernova remnants

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979acasn..20..393m&link_type=abstract

Acta Astronomica Sinica, vol. 20, Dec. 1979, p. 393-397. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

1

Interstellar Radiation, Radio Emission, Supernova Remnants, X Ray Astronomy, Astronomical Models, Brightness, Cosmology, Interstellar Matter, Neutron Stars

Scientific paper

According to the usual blast model of SNRs, a set of correlated formulae for known-age SNRs were deduced. Using X-ray information and the ages of SNRs, the basic physical parameters of a SNR are determined by these formulae which were applied to the sources of SN185, SN1006 and SN1054 to evaluate three sets of SNR's parameters, in which the distances of the SNRs agree with the ancient apparent brightness data. It is emphasized that the density of the interstellar medium has an important effect on the nature of radio emissions, and this will be helpful for the theoretical interpretation of the physical states of SNRs.

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