Supernova remnants - What do they tell us about massive star evolution and the interstellar medium

Details Supernova remnants - What do they tell us about massive star evolution and the interstellar medium Supernova remnants - What do they tell us about massive star evolution and the interstellar medium

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978msngr..13...20d&link_type=abstract

ESO Messenger, June 1978, p. 20-23.

Astronomy and Astrophysics

Astronomy

Interstellar Matter, Stellar Evolution, Supernova Remnants, Abundance, Line Spectra, Pulsars, Radio Astronomy, X Ray Astronomy

Scientific paper

Present-day knowledge of supernova remnants (SNRs) is reviewed. Attention is given to the four phases in the dynamical evolution of an SNR shell, expansion ages of galactic SNRs, abundance determinations for galactic and Magellanic Cloud SNRs, and the frequency of supernova explosions in the Galaxy and the Large Magellanic Cloud. The individual SNRs discussed include the Crab Nebula, the Cygnus Loop, Cas A, the Monoceros SNR, the Tycho and Vela SNRs, SN 1006, W44, and N 63 A and N 132 D in the Large Magellanic Cloud.

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