THE DUST BUDGET OF THE SMALL MAGELLANIC CLOUD: ARE ASYMPTOTIC GIANT BRANCH STARS THE PRIMARY DUST SOURCE AT LOW METALLICITY? (2012)
Attributed to:
Stellar Astrophysics at Keele
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/0004-637x/748/1/40
Publication URI: http://dx.doi.org/10.1088/0004-637x/748/1/40
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1
ISSN: 0004-637X