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The mass-loss rates of red supergiants at low metallicity: detection of rotational CO emission from two red supergiants in the Large Magellanic Cloud (2016)

First Author: Matsuura M

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/10.1093/mnras/stw1853

Publication URI: http://dx.doi.org/10.1093/mnras/stw1853

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3