activity
20222025
most citedGrids of stellar models with rotation VI: Models from 0.8 to 120 at a metallicity Z = 0.006

68 citations · 95 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2025★ 10 cited

pySTARBURST99: The Next Generation of STARBURST99

Calum Hawcroft, Claus Leitherer, Oskar Arangure +8

STARBURST99 is a population synthesis code tailored to predict the integrated properties or observational characteristics of star-forming galaxies. Here we present an update to STA…

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★ 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.SR2022★ 13 cited

Very massive star winds as sources of the short-lived radioactive isotope Al

S. Martinet, G. Meynet, D. Nandal +7

The Al short-lived radioactive nuclide is the source of the observed galactic diffuse -ray emission at 1.8 MeV. While different sources of Al have been explored, s…

astro-ph.GA2022★ 68 cited

Grids of stellar models with rotation VI: Models from 0.8 to 120 at a metallicity Z = 0.006

Patrick Eggenberger, Sylvia Ekström, Cyril Georgy +14

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 are a key…