Grids of stellar models with rotation VI. Models from 0.8 to 120 M-circle dot at a metallicity Z=0.006

• Main Authors: Eggenberger, Patrick, Ekstroem, Sylvia, Georgy, Cyril, Martinet, Sebastien, Pezzotti, Camilla, Nandal, Devesh, Meynet, Georges, Buldgen, Gael, Salmon, Sebastien, Haemmerle, Lionel, Maeder, Andre, Hirschi, Raphael, Yusof, Norhasliza, Groh, Jose, Farrell, Eoin, Murphy, Laura, Choplin, Arthur
• Format: Article
• Published: Edp Sciences S A 2021
• Subjects: QC Physics
• Online Access: http://eprints.um.edu.my/34597/
• Institution: Universiti Malaya

Context. Grids of stellar models, computed with the same physical ingredients, allow one to study the impact of a given physics on a broad range of initial conditions and they are a key ingredient for modeling the evolution of galaxies. Aims. We present here a grid of single star models for masses b...