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

Simple item page
dc.contributor.authorGroenewegen, M A T
dc.contributor.authorVlemmings, W H T
dc.contributor.authorMarigo, P
dc.contributor.authorSloan, G C
dc.contributor.authorDecin, L
dc.contributor.authorFeast, M W
dc.contributor.authorGoldman, S R
dc.contributor.authorJusttanont, K
dc.contributor.authorKerschbaum, F
dc.contributor.authorMatsuura, M
dc.contributor.authorMcDonald, I
dc.contributor.authorOlofsson, H
dc.contributor.authorSahai, R
dc.contributor.authorvan Loon, J Th
dc.contributor.authorWood, P R
dc.contributor.authorZijlstra, A A
dc.contributor.authorBernard-Salas, J
dc.contributor.authorBoyer, M L
dc.contributor.authorGuzman-Ramirez, L
dc.contributor.authorJones, O C
dc.contributor.authorLagadec, E
dc.contributor.authorMeixner, M
dc.contributor.authorRawlings, M G
dc.contributor.authorSrinivasan, S
dc.date.accessioned2021-10-08T06:20:07Z
dc.date.available2021-10-08T06:20:07Z
dc.date.issued2016
dc.description.abstractContext. 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.
dc.identifier.apacitationGroenewegen, M. A. T., Vlemmings, W. H. T., Marigo, P., Sloan, G. C., Decin, L., Feast, M. W., ... Srinivasan, S. (2016). The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud. <i>Astronomy and Astrophysics</i>, 596(4), A50 - 177. http://hdl.handle.net/11427/34208en_ZA
dc.identifier.chicagocitationGroenewegen, M A T, W H T Vlemmings, P Marigo, G C Sloan, L Decin, M W Feast, S R Goldman, et al "The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud." <i>Astronomy and Astrophysics</i> 596, 4. (2016): A50 - 177. http://hdl.handle.net/11427/34208en_ZA
dc.identifier.citationGroenewegen, 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. <i>Astronomy and Astrophysics.</i> 596(4):A50 - 177. http://hdl.handle.net/11427/34208en_ZA
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.ris TY - Journal Article AU - Groenewegen, M A T AU - Vlemmings, W H T AU - Marigo, P AU - Sloan, G C AU - Decin, L AU - Feast, M W AU - Goldman, S R AU - Justtanont, K AU - Kerschbaum, F AU - Matsuura, M AU - McDonald, I AU - Olofsson, H AU - Sahai, R AU - van Loon, J Th AU - Wood, P R AU - Zijlstra, A A AU - Bernard-Salas, J AU - Boyer, M L AU - Guzman-Ramirez, L AU - Jones, O C AU - Lagadec, E AU - Meixner, M AU - Rawlings, M G AU - Srinivasan, S AB - 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. DA - 2016 DB - OpenUCT DP - University of Cape Town IS - 4 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2016 SM - 0004-6361 SM - 1432-0746 T1 - The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud TI - The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud UR - http://hdl.handle.net/11427/34208 ER - en_ZA
dc.identifier.urihttp://hdl.handle.net/11427/34208
dc.identifier.vancouvercitationGroenewegen MAT, Vlemmings WHT, Marigo P, Sloan GC, Decin L, Feast MW, et al. The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud. Astronomy and Astrophysics. 2016;596(4):A50 - 177. http://hdl.handle.net/11427/34208.en_ZA
dc.language.isoeng
dc.publisher.departmentDepartment of Astronomy
dc.publisher.facultyFaculty of Science
dc.sourceAstronomy and Astrophysics
dc.source.journalissue4
dc.source.journalvolume596
dc.source.paginationA50 - 177
dc.source.urihttps://dx.doi.org/10.1051/0004-6361/201629590
dc.subject.otherstars: AGB and post-AGB
dc.subject.otherstars: winds, outflows
dc.subject.otherradio continuum: stars
dc.subject.otherstars: winds
dc.subject.otheroutflows
dc.titleThe ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud
dc.typeJournal Article
uct.type.publicationResearch
uct.type.resourceJournal Article
Files
Original bundle
Now showing 1 - 1 of 1
Thumbnail Image
Name:
GroenewegenMAT_ALMA_detectionC_2016.pdf
Size:
748.66 KB
Format:
Adobe Portable Document Format
Description:
Download
Collections
Journal Articles