Grids of stellar models with rotation VI. Models from 0.8 to 120 M-circle dot at a metallicity Z=0.006
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...
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Main Authors: | , , , , , , , , , , , , , , , , |
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Format: | Article |
Published: |
Edp Sciences S A
2021
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Subjects: | |
Online Access: | http://eprints.um.edu.my/34597/ |
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Institution: | Universiti Malaya |