Grids of stellar models with rotation - V. Models from 1.7 to 120 M? at zero metallicity (2021)

First Author: Murphy L
Attributed to:  Cosmic Impact of Massive Stars: Convective Mixing and Mass Loss funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa3803

Publication URI: http://dx.doi.org/10.1093/mnras/staa3803

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2