Why binary interaction does not necessarily dominate the formation of Wolf-Rayet stars at low metallicity (2020)

First Author: Shenar T
Attributed to:  Cosmic Impact of Massive Stars: Mass Loss and Mixing funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201936948

Publication URI: http://dx.doi.org/10.1051/0004-6361/201936948

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics