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Sodium content as a predictor of the advanced evolution of globular cluster stars

Campbell, Simon W; D’Orazi , V; Yong, David; Constantino, Thomas N; Lattanzio, John; Stancliffe, Richard; Angelou, G C; Wylie de Boer, Elizabeth; Grundahl, Frank

Description

The asymptotic giant branch (AGB) phase is the final stage of nuclear burning for low-mass stars. Although Milky Way globular clusters are now known to harbour (at least) two generations of stars, they still provide relatively homogeneous samples of stars

CollectionsANU Research Publications
Date published: 2013
Type: Journal article
URI: http://hdl.handle.net/1885/73011
Source: Nature
DOI: 10.1038/nature12191

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