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Low Mass Asymptotic Giant Branch Evolution
Published online by Cambridge University Press: 25 April 2016
Extract
The evolution of asymptotic giant branch (AGB) stars as a function of mass and composition has been studied by Becker and Iben (1979, 1980) for M≥3 M⊙. The results from calculations like these may be used to provide input data for calculations of synthetic AGB star populations, as has been done by Wood and Cahn (1977), Iben (1981) and Renzini and Voli (1981).
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- Copyright © Astronomical Society of Australia 1984