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20212025
most citedGrids of stellar models with rotation VII: Models from 0.8 to 300 M at super-solar metallicity (Z = 0.020)

50 citations · 193 across the 12 of their papers we have counts for

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7 papers · 1 filter

astro-ph.SR2025★ 7 cited

The fate of rotating massive stars across cosmic times

R. Hirschi, K. Goodman, G. Meynet +9

The initial mass and metallicity of stars both have a strong impact on their fate. Stellar axial rotation also has a strong impact on the structure and evolution of massive stars.…

astro-ph.SR2025

Fluorine production in He-burning regions of massive stars during cosmic history

Sophie Tsiatsiou, Georges Meynet, Eoin Farrell +11

The origin of fluorine is still a debated question. AGB stars synthesise this element and likely contribute significantly to its synthesis in the present-day Universe. However, it…

astro-ph.SR2024★ 1 cited

Grids of stellar models with rotation VIII: Models from 1.7 to 500 at metallicity

Yves Sibony, Kendall G. Shepherd, Norhasliza Yusof +12

Grids of stellar evolution models with rotation using the Geneva stellar evolution code (Genec) have been published for a wide range of metallicities. We introduce the last remaini…

astro-ph.SR2024★ 24 cited

Rapidly rotating Population III stellar models as a source of primary nitrogen

Sophie Tsiatsiou, Yves Sibony, Devesh Nandal +12

The first stars might have been fast rotators. This would have important consequences for their radiative, mechanical and chemical feedback. We discuss the impact of fast initial r…

astro-ph.SR2023★ 15 cited

The impact of convective criteria on the properties of massive stars

Yves Sibony, Cyril Georgy, Sylvia Ekström +1

We study the differences between models computed with Ledoux and Schwarzschild criteria on the internal structure, evolutionary track in the Hertzsprung-Russell diagram (HRD), life…

astro-ph.SR2022★ 17 cited

Impact of Population III homogeneous stellar evolution on early cosmic reionisation

Yves Sibony, Boyuan Liu, Charlotte Simmonds +2

Context: Population III (Pop III) stars may be fast rotating. An expected consequence of fast rotation is strong internal mixing that deeply affects their evolutionary tracks in th…

astro-ph.SR2022★ 50 cited

Grids of stellar models with rotation VII: Models from 0.8 to 300 M at super-solar metallicity (Z = 0.020)

Norhasliza Yusof, Raphael Hirschi, Patrick Eggenberger +11

We present a grid of stellar models at super-solar metallicity (Z = 0.020) extending the previous grids of Geneva models at solar and sub-solar metallicities. A metallicity of Z =…