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- W90802392 abstract "We describe in a brief form recent evolution calculations for low mass stars having solar-like initial composition up to their AGB phase. In this contribution we present the evolution of a 2 M star which evolves through the core helium flash before reaching the AGB phase and compare it to the evolution of a 3 M star which avoids the core Helium flash. In particular, we illustrate the effect of neutrino losses on the onset of thermal pulsation and the duration of the thermal pulses. Some characteristics of the core helium flash of the 2 M star are presented." @default.
- W90802392 created "2016-06-24" @default.
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- W90802392 date "2006-01-01" @default.
- W90802392 modified "2023-09-23" @default.
- W90802392 title "Comments on the evolution of AGB stars" @default.
- W90802392 hasPublicationYear "2006" @default.
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