S´ebastien Martinet

activity

20222025

most citedGrids of stellar models with rotation VI: Models from 0.8 to 120

M_{⊙}

at a metallicity Z = 0.006

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

collaborators

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2 papers · 1 filter

astro-ph.SR2022★ 13 cited

Very massive star winds as sources of the short-lived radioactive isotope $^{26}$ Al

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

The $^{26}$ Al short-lived radioactive nuclide is the source of the observed galactic diffuse $γ$ -ray emission at 1.8 MeV. While different sources of $^{26}$ Al have been explored, s…

astro-ph.GA2022★ 68 cited

Grids of stellar models with rotation VI: Models from 0.8 to 120 $M_{⊙}$ 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…

Very massive star winds as sources of the short-lived radioactive isotope 26Al

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

Very massive star winds as sources of the short-lived radioactive isotope $^{26}$ Al

Grids of stellar models with rotation VI: Models from 0.8 to 120 $M_{⊙}$ at a metallicity Z = 0.006