Interaction of Supernovae with Circumstellar Matter

Chevalier, Roger A.

doi:10.1007/978-1-4612-3286-5_5

Interaction of Supernovae with Circumstellar Matter

Roger A. Chevalier

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Abstract

Stars of essentially all masses are known to lose mass during their evolution. The mass loss characteristics at any time are determined by the evolutionary status of the star. The region around a star that is modified by these processes is referred to as the circumstellar medium. In addition to mass loss from a single star, mass transfer and mass loss in a binary system may play a role in determining the circumstellar environment.

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Roger A. Chevalier
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Editors and Affiliations

Department of Physics, New Mexico Institute of Mining and Technology, Socorro, NM, 87801, USA
Albert G. Petschek
Los Alamos National Laboratory, Mail Stop D434, Los Alamos, NM, 87545, USA
Albert G. Petschek

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Chevalier, R.A. (1990). Interaction of Supernovae with Circumstellar Matter. In: Petschek, A.G. (eds) Supernovae. Astronomy and Astrophysics Library. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-3286-5_5

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DOI: https://doi.org/10.1007/978-1-4612-3286-5_5
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