THE INFRARED SPECTRAL PROPERTIES OF MAGELLANIC CARBON STARS (2016)
Attributed to:
Dust formation by supernovae and asymptotic giant branch stars
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/0004-637x/826/1/44
Publication URI: http://dx.doi.org/10.3847/0004-637x/826/1/44
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1