The interaction of supernovae with circumstellar bubbles

Details The interaction of supernovae with circumstellar bubbles The interaction of supernovae with circumstellar bubbles

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...344..332c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 344, Sept. 1, 1989, p. 332-340.

Astronomy and Astrophysics

Astronomy

106

Stellar Envelopes, Stellar Winds, Supernova Remnants, Supernovae, Radio Sources (Astronomy), Shock Waves, Stellar Evolution, Stellar Mass, Supernova 1987A, X Ray Sources

Scientific paper

This paper examines the interaction of a massive star supernova with the shell created by the fast wind from a blue supergiant, either in the main-sequence phase or in a late evolutionary phase. Making a number of idealizations, the general features of shell interaction are described by semianalytical solutions. The expected properties of the supernova and its environment are discussed, and the hydrodynamics of the interaction is described. It is found that, typically, the shock traversal occurs before the energy transfer is significant. Applications of the model to observed objects are considered, with special attention given to the interaction of SN 1987A with its circumstellar shell, which is expected to occur within decades.

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