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- W1659380935 abstract "Supernova 1993 J exploded in the nearby spiral galaxy M81. Its initial spectrum contained hydrogen lines and therefore it was classified as a Type II supernova. However, subsequent disappearance of hydrogen lines and appearance of helium lines made it similar to a type Ib supernova. Radio emission was detected from SN 1993 J shortly after the first peak in optical brightness. In this paper we present a model for the observed radio radiation that involves the interaction of a collisionless shock front generated by the supernova ejecta and a stellar wind produced by the progenitor supergiant. We discuss electron acceleration, magnetic field generation and interpret an observed break in the radio spectrum." @default.
- W1659380935 created "2016-06-24" @default.
- W1659380935 creator A5042287077 @default.
- W1659380935 date "2000-01-01" @default.
- W1659380935 modified "2023-09-27" @default.
- W1659380935 title "Radio emission from supernova 1993 J" @default.
- W1659380935 cites W1541466590 @default.
- W1659380935 doi "https://doi.org/10.1063/1.1291710" @default.
- W1659380935 hasPublicationYear "2000" @default.
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