Thermal Pulses and Planetary Nebula Ejection
نویسندگان
چکیده
منابع مشابه
Very Late Thermal Pulses Influenced by Accretion in Planetary Nebulae
We consider the possibility that a mass of ∼ 10 − 10M⊙ flows back from the dense shell of planetary nebulae and is accreted by the central star during the planetary nebula phase. This backflowing mass is expected to have a significant specific angular momentum even in (rare) spherical planetary nebulae, such that a transient accretion disk might be formed. This mass might influence the occurren...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1993
ISSN: 0074-1809
DOI: 10.1017/s0074180900171025