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An AGB Star with a Thick Circumstellar Shell
Mould, Jeremy1; Durre, Mark1; Uddin, Syed2; Wang, Lifan3,4
2020-04-01
Source PublicationPUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
ISSN0004-6280
Volume132Issue:1010Pages:5
Corresponding AuthorMould, Jeremy(jmould@swin.edu.au)
AbstractThe Asymptotic Giant Branch is the terminal phase of red giant evolution with timescales of millions of years and a total mass lost from the star that is a significant fraction of the initial mass. Investigation of one of these stars, WISEA J173046.10-344455.5, a kpc in the direction of the center of the Galaxy, reveals a cool oxygen rich star with a dust shell of blackbody temperature 1305 K.
Keywordstars AGB and post-AGB stars mass-loss stars variables general
DOI10.1088/1538-3873/ab77d8
WOS KeywordASYMPTOTIC GIANT BRANCH ; LARGE-MAGELLANIC-CLOUD ; RED GIANTS ; DUST ; EVOLUTION ; OUTBURST ; LIBRARY ; SAGE
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000521364400001
PublisherIOP PUBLISHING LTD
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/35887
Collection中国科学院紫金山天文台
Corresponding AuthorMould, Jeremy
Affiliation1.Swinburne Univ, Ctr Astrophys & Supercomp, POB 218, Hawthorn, Vic 3122, Australia
2.Carnegie Observ, 813 Santa Barbara St, Pasadena, CA USA
3.Texas A&M Univ, Mitchell Inst Fundamental Phys & Astron, College Stn, TX 77843 USA
4.Purple Mt Observ, Nanjing 201008, Jiangsu, Peoples R China
Recommended Citation
GB/T 7714
Mould, Jeremy,Durre, Mark,Uddin, Syed,et al. An AGB Star with a Thick Circumstellar Shell[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,2020,132(1010):5.
APA Mould, Jeremy,Durre, Mark,Uddin, Syed,&Wang, Lifan.(2020).An AGB Star with a Thick Circumstellar Shell.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,132(1010),5.
MLA Mould, Jeremy,et al."An AGB Star with a Thick Circumstellar Shell".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 132.1010(2020):5.
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