Mass loss from highly evolved stars
نویسندگان
چکیده
منابع مشابه
Dust production and mass loss in cool evolved stars
Following the red giant branch phase and the subsequent core He-burning phase, the lowto intermediate-mass stars (0.8 < M/M < 8) begin to ascend the asymptotic giant branch (AGB). Pulsations levitate material from the stellar surface and provide density enhancements and shocks, which can encourage dust formation and re-processing. The dust composition depends on the atmospheric chemistry (abund...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1984
ISSN: 0074-1809
DOI: 10.1017/s0074180900030941