Models of quiescent stellar microwave emission
Identifieur interne : 000940 ( Main/Exploration ); précédent : 000939; suivant : 000941Models of quiescent stellar microwave emission
Auteurs : E. Gary [États-Unis]Source :
- Lecture Notes in Physics [ 0075-8450 ] ; 1986.
Abstract
Abstract: Models for gyrosynchrotron emission from thermal electrons in dMe stellar coronae are developed using the formula for electron emissivity given by Robinson and Melrose (1984). The most physically plausible model also closely fits VIA observations. A comparison of this model to the observations is presented.
Url:
DOI: 10.1007/3-540-16763-3_182
Affiliations:
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