The Magellanic Cloud supernova remnants

Details The Magellanic Cloud supernova remnants The Magellanic Cloud supernova remnants

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..271d&link_type=abstract

IN: Structure and evolution of the Magellanic Clouds; Proceedings of the Symposium, Tuebingen, West Germany, September 5-8, 1983

Mathematics

2

Magellanic Clouds, Supernova Remnants, Cosmochemistry, Interstellar Matter, Oxygen Spectra, Shock Waves, Spectrophotometry, Stellar Evolution, Stellar Mass, X Ray Sources

Scientific paper

The first supernova remnant (SNR) in the Magellanic Clouds was discovered by Mathewson and Healey (1964). Surveys for SNR in the Magellanic Clouds are discussed, taking into account the selection procedure initially used, current optical selection criteria for SNR, the launching of the Einstein Observatory, and the information obtainable by a detailed study of the discovered SNR. Attention is also given to the oxygen-rich SNR, the nonradiative shock SNR, the evolved radiative SNR, and conclusions based on the obtained results.

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