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Grids of stellar models with rotation VI. Models from 0.8 to 120 M ? at a metallicity Z = 0.006 (2021)

First Author: Eggenberger P

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/10.1051/0004-6361/202141222

Publication URI: http://dx.doi.org/10.1051/0004-6361/202141222

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics