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The Special Case of ω Centauri

Published online by Cambridge University Press:  30 March 2016

John E. Norris*
Affiliation:
Research School of Astronomy & Astrophysics, Institute of Advanced Studies, The Australian National University, Mount Stromlo Observatory, Cotter Road, Weston ACT 2611, Australia

Abstract

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ω Cen is unique among the Galactic globular clusters. It exhibits not only classical mixing signatures, but also those of primordial chemical enrichment by both massive and intermediate-mass stars: the abundances of all elements vary, not just those of the C, N, O, Na, Mg, and Al. The challenge is to disentangle the roles of mixing and primordial phenomena. We discuss here what sets ω Cen apart from the other clusters.

Type
II. Joint Discussions
Copyright
Copyright © Astronomical Society of Pacific 2002

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