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Low Mass Asymptotic Giant Branch Evolution

Published online by Cambridge University Press:  25 April 2016

J. C. Lattanzio
J. C. Lattanzio*
Affiliation:
Department of Mathematics, Monash University
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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).

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 4 , 1984 , pp. 498 - 500
Copyright
Copyright © Astronomical Society of Australia 1984

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References

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