Skip navigation
Skip navigation

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

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

Description

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

Download

File Description SizeFormat Image
01_Ventura_The_Large_Magellanic_Cloud_as_2015.pdf663.04 kBAdobe PDF    Request a copy


Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  23 August 2018/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator