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The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud

Groenewegen, M. A. T.; Vlemmings, W. H. T.; Marigo, P.; Sloan, G. C.; Decin, L.; Feast, M. W.; Goldman, S. R.; Justtanont, K.; Kerschbaum, F.; Matsuura, M.; McDonald, I.; Olofsson, H.; Sahai, R.; van Loon, J. Th.; Wood, P. R.; Zijlstra, A. A.; Bernard-Salas, J.; Boyer, M. L.; Guzman-Ramirez, L.; Jones, O. C.; Lagadec, Eric; Meixner, M.; Rawlings, M. G.; Srinivasan, S.

Description

Context: Low- and intermediate-mass stars lose most of their stellar mass at the end of their lives on the asymptotic giant branch (AGB). Determining gas and dust mass-loss rates (MLRs) is important in quantifying the contribution of evolved stars to the enrichment of the interstellar medium. Aims: Attempt to, for the first time, spectrally resolve CO thermal line emission in a small sample of AGB stars in the Large Magellanic Cloud. Methods: ALMA was used to observe 2 OH/IR stars and 4...[Show more]

CollectionsANU Research Publications
Date published: 2016-11-29
Type: Journal article
URI: http://hdl.handle.net/1885/114186
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/201629590

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