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Hot Bottom Burning in a 5 M⊙ Model

Published online by Cambridge University Press:  25 April 2016

John C. Lattanzio
John C. Lattanzio*
Affiliation:
Mathematics Department, Monash University, Clayton VIC 3168
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Abstract

This paper presents recent stellar evolutionary calculations of the Asymptotic Giant Branch evolution of a 5M⊙ model. It is found that temperatures at the base of the convective envelope reach up to almost 100 million degrees, high enough for much nucleo-synthesis to occur. Some implications are discussed briefly.

Type
Galactic and Stellar
Information
Publications of the Astronomical Society of Australia , Volume 10 , Issue 2 , 1992 , pp. 120 - 121
Copyright
Copyright © Astronomical Society of Australia 1992

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