Grids of stellar models with rotation I. Models from 0.8 to 120  M ? at solar metallicity ( Z = 0.014)? (2012)

First Author: Ekström S
Attributed to:  Stellar Astrophysics at Keele funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201117751

Publication URI: http://dx.doi.org/10.1051/0004-6361/201117751

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics