📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

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

Attributed to: Gas, dust and stars: the life cycle of galaxies funded by STFC

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