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Globular cluster abundances: the role of asymptotic giant branch stars

Published online by Cambridge University Press:  18 January 2010

Amanda I. Karakas
Amanda I. Karakas*
Affiliation:
Mount Stromlo Observatory, Australian National University, Weston Creek ACT 2611, Australia email: [email protected]
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Abstract

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One of the more popular theories to account for the abundance anomalies in globular cluster stars is the ‘self-pollution scenario,’ where the polluters were a previous generation of intermediate-mass asymptotic giant branch (AGB) stars. This idea has proved attractive because: (i) the hot-bottom burning experienced by these objects qualitatively provides an ideal proton-capture environment to produce helium and convert C and O to N, Ne to Na and Mg to Al, and (ii) the slow winds from these stars allow their retention by the cluster's gravitational potential. New stellar yields from low-metallicity AGB models are presented and compared to abundances derived in globular clusters. We also discuss external pollution and inhomogeneous-pollution models that use AGB stars as polluters. Current models of AGB stars cannot match all observational features of globular cluster stars. However, stellar modelling uncertainties are considerable and suggest AGB stars should not be ruled out just yet.

Keywords

stars: abundancesstars: AGB and post-AGBglobular clusters: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S266: Star clusters: basic galactic building blocks throughout time and space , August 2009 , pp. 161 - 168
Copyright
Copyright © International Astronomical Union 2010

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