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Grids of stellar models with rotation VI: Models from 0.8 to 120 $M_odot$ at a metallicity Z = 0.006. (arXiv:2201.12262v1 [astro-ph.GA])
- Volume 17, Issue 5 - article #5
- Patrick Eggenberger, Sylvia Ekström, Cyril Georgy, Sébastien Martinet, Camilla Pezzotti, Devesh Nandal, Georges Meynet, Gaël Buldgen, Sébastien Salmon, Lionel Haemmerlé, André, Maeder, Raphael Hirschi, Norhasliza Yusof, José, Groh, Eoin Farrell, Laura Murphy, Arthur Choplin
- http://arxiv.org/abs/2201.12262
Ionizing photon production of Population III stars: effects of rotation, convection, and initial mass function. (arXiv:2105.06900v2 [astro-ph.SR] UPDATED)
- Volume 16, Issue 28 - article #2
- Laura J. Murphy, Jose H. Groh, Eoin Farrell, Georges Meynet, Sylvia Ekström, Sophie Tsiatsiou, Alexander Hackett, Sébastien Martinet
- http://arxiv.org/abs/2105.06900

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