The mass-loss return from evolved stars to the Large Magellanic Cloud III. Dust properties for carbon-rich asymptotic giant branch stars (2010)

First Author: Srinivasan S

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201014991

Publication URI: http://dx.doi.org/10.1051/0004-6361/201014991

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics