Properties of supernova remnants at known distances. III - Energy content

Details Properties of supernova remnants at known distances. III - Energy content Properties of supernova remnants at known distances. III - Energy content

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...192..299b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 192, no. 1-2, March 1988, p. 299-312.

Astronomy and Astrophysics

Astronomy

9

Astronomical Spectroscopy, Stellar Envelopes, Supernova Remnants, Thermal Energy, X Ray Sources, Kinetic Energy, Radio Sources (Astronomy), Relativistic Particles, Sulfur

Scientific paper

The energy content of shell-type SNRs at known distances was determined from observations of the emission in the radio continuum, X-rays, and forbidden S II lines. A nearly constant radio surface brightness during the observable part of the evolution of an SNR is implied. The thermal energy seen in X-rays was calculated for remnants with known shock temperature.

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