activity
20032026
most citedGrids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)

1.7k citations · 9.3k across the 137 of their papers we have counts for

collaborators

141 papers

astro-ph.GA2026

Stellar Yields of Rapidly Rotating Population III Stars for the High Redshift Universe

Devesh Nandal, Konstantinos Topalakis, Vasilisa Sergienko +6

JWST has revealed rapid nitrogen enrichment in high redshift galaxies, renewing the need for stellar yields that follow metal free stars beyond the main sequence and across their f…

astro-ph.SR2025

Apsidal Motion in O-Star Binaries: GENEC rotating binary models put to the k2-test

Sophie Rosu, Luca Sciarini, Sylvia Ekström +1

Unveiling massive stars' internal structure and the physical origin and efficiency of the internal mixing processes? It is now possible using the apsidal motion rate in close eccen…

astro-ph.SR2025★ 4 cited

The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity

Erin R. Higgins, Jorick S. Vink, Raphael Hirschi +2

The chemical feedback from stellar winds in low metallicity (Z) environments is key for understanding the evolution of globular clusters and the early Universe. With disproportiona…

astro-ph.SR2024★ 4 cited

Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network

Adam Griffiths, Miguel-Á Aloy, Raphael Hirschi +6

Stars with initial mass above roughly 8 solar masses will evolve to form a core made of iron group elements at which point no further exothermic nuclear reactions between charged n…

astro-ph.SR2024

New Wolf-Rayet wind yields and nucleosynthesis of Helium stars

Erin R. Higgins, Jorick S. Vink, Raphael Hirschi +2

Strong metallicity-dependent winds dominate the evolution of core He-burning, classical Wolf-Rayet (cWR) stars, which eject both H and He-fusion products such as 14N, 12C, 16O, 19F…

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…