Mass conservation and rapid mass loss on the main sequence
نویسندگان
چکیده
منابع مشابه
Theoretical mass loss rates of cool main - sequence stars
Context. The stellar mass loss rate is important for the rotational evolution of a star and for its interaction with the circumstellar environment. The analysis of astrospheric absorption features enables an empirical determination of mass loss rates of cool stars other than the Sun. Aims. We develop a model for the wind properties of cool main-sequence stars, which comprises their wind ram pre...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1979
ISSN: 0074-1809
DOI: 10.1017/s0074180900013759