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The Large Magellanic Cloud as a laboratory for hot bottom burning in massive asymptotic giant branch stars

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Ventura, P; Karakas, Amanda; Dell'Agli, F; Boyer, M L; Garcia-Hernandez, D. A.; Di Criscienzo, M; Schneider, R

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We use Spitzer observations of the rich population of asymptotic giant branch (AGB) stars in the Large Magellanic Cloud (LMC) to test models describing the internal structure and nucleosynthesis of the most massive of these stars, i.e. those with initial

CollectionsANU Research Publications
Date published: 2015
Type: Journal article
URI: http://hdl.handle.net/1885/70629
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1093/mnras/stv918

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