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

Journal Article

2016

Permanent link to this Item
http://hdl.handle.net/11427/34208
Files
GroenewegenMAT_ALMA_detectionC_2016.pdf (748.66 KB)
Authors
Groenewegen, M A T
Vlemmings, W H T
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
Marigo, P
Lagadec, E
Meixner, M
Rawlings, M G
Srinivasan, S
Sloan, G C
Decin, L
Feast, M W
Goldman, S R
Justtanont, K
Kerschbaum, F
Matsuura, M
Journal Title

Astronomy and Astrophysics

Link to Journal
https://dx.doi.org/10.1051/0004-6361/201629590
Journal ISSN
Volume Title
Publisher
Publisher
Department
Department of Astronomy
Faculty
Faculty of Science
License
Series
Abstract
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.
Description
Keywords
stars: AGB and post-AGB
stars: winds, outflows
radio continuum: stars
stars: winds
outflows

Reference:

Groenewegen, M.A.T., Vlemmings, W.H.T., Marigo, P., Sloan, G.C., Decin, L., Feast, M.W., Goldman, S.R. & Justtanont, K. et al. 2016. The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud. Astronomy and Astrophysics. 596(4):A50 - 177. http://hdl.handle.net/11427/34208

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