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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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Date

2015

Authors

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

Journal Title

Journal ISSN

Volume Title

Publisher

Blackwell Publishing Ltd

Abstract

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

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Keywords

Citation

URI

http://hdl.handle.net/1885/70629

Collections

ANU Research Publications

Source

Monthly Notices of the Royal Astronomical Society

Type

Journal article

Book Title

Entity type

Access Statement

License Rights

DOI

10.1093/mnras/stv918

Restricted until

2037-12-31

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01_Ventura_The_Large_Magellanic_Cloud_as_2015.pdf (663.04 KB)

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