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Collision-induced mass loss and mass gain on an extremely massive star : An analytical approach and a static proto-globular cluster test-caseAstronomy & astrophysics
accessLevelRestricted
2025 22 0
Using 26 Al to detect ongoing self-enrichment in young massive star clustersMonthly notices of the Royal Astronomical Society
accessLevelPublic
2024 30 420
N-enhancement in GN-z11: First evidence for supermassive stars nucleosynthesis in proto-globular clusters-like conditions at high redshift?Astronomy & astrophysics
accessLevelPublic
2023 26 255
Can the stellar dynamical tide destabilize the resonant chains of planets formed in the disk?Proceedings of the International Astronomical Union, Volume 18, Symposium S382: Complex Planetary Systems II: Latest Methods for an Interdisciplinary Approach
accessLevelPublic
2022 1 0
Grids of stellar models with rotation. I: Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)Astronomy & astrophysics
accessLevelPublic
2012 388 1,115
The Geneva stellar evolution codeAstrophysics and Space Science
accessLevelPublic
2008 566 696
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