Output details
9 - Physics
Keele University
Grids of stellar models with rotation I. Models from 0.8 to 120 M-circle dot at solar metallicity (Z=0.014)
Hirschi (with his PhD student Urs Frischknecht) contributed in several ways to the project "Grids of Stellar Models with Rotation", which includes models at several metallicities, Z: 0.02 (super-solar), 0.014 (solar), 0.006 (LMC) and 0.002 (SMC). Hirschi contributed to the development of the Geneva stellar evolution code, especially for the modelling of advanced stellar stages, as well as the automation of the calculations. Hirschi is in charge of the calculations at Z=0.02. This paper at Z=0.014 is the first of a series for this large project; Hirschi contributed to the analysis and the paper writing.