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Production of Aluminium and the Heavy Magnesium Isotopes in Asymptotic Giant Branch Stars

Published online by Cambridge University Press:  05 March 2013

A. I. Karakas  and
J. C. Lattanzio
A. I. Karakas*
Affiliation:
School of Mathematical Sciences, Monash University, Wellington Road, Clayton, Vic 3800, Australia.
J. C. Lattanzio
Affiliation:
School of Mathematical Sciences, Monash University, Wellington Road, Clayton, Vic 3800, Australia.
*
[email protected]
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Abstract

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We investigate the production of aluminium and magnesium in asymptotic giant branch models covering a wide range in mass and composition. We evolve models from the pre-main sequence, through all intermediate stages, to near the end of the thermally-pulsing asymptotic giant branch phase. We then perform detailed nucleosynthesis calculations from which we determine the production of the magnesium and aluminium isotopes as a function of the stellar mass and composition. We present the stellar yields of sodium and the magnesium and aluminium isotopes. We discuss the abundance predictions from the stellar models in reference to abundance anomalies observed in globular cluster stars.

Keywords

stars: AGB and post-AGBstars: abundancesstars: interiorsstars: low massISM: abundances
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 20 , Issue 3 , 2003 , pp. 279 - 293
Copyright
Copyright © Astronomical Society of Australia 2003

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