The dust budget of the small magellanic cloud: Are asymptotic giant branch stars the primary dust source at low metallicity?

Astrophysical Journal

Volumn 748, Issue 1, 2012, Pages

  Boyer, M L ^a   Srinivasan, S ^b   Riebel, D ^c   McDonald, I ^d   Van Loon, J Th ^e   Clayton, G C ^f   Gordon, K D ^a   Meixner, M ^a   Sargent, B A ^a   Sloan, G C ^g  

^a STScI   (United States)

^b INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d UNIVERSITY OF MANCHESTER   (United Kingdom)

^e KEELE UNIVERSITY   (United Kingdom)

^f LOUISIANA STATE UNIVERSITY   (United States)

^g Department of Obstetrics Gynecology   (United States)

Author keywords

dust, extinction; Magellanic Clouds; stars: AGB and post AGB; supernovae: general

Indexed keywords

EID: 84857951323     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/748/1/40     Document Type: Article

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