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20152025
most citedGrids of stellar models with rotation VI: Models from 0.8 to 120 at a metallicity Z = 0.006

68 citations · 288 across the 10 of their papers we have counts for

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Showing 2022Show all

5 papers · 1 filter

astro-ph.GA2022★ 26 cited

Direct collapse of exceptionally heavy black holes in the merger-driven scenario

Lorenz Zwick, Lucio Mayer, Lionel Haemmerlé +1

We revisit the conditions present in supermassive discs (SMDs) formed by the merger of gas-rich, metal-enriched galaxies at red-shift . We find that SMDs naturally form h…

astro-ph.SR2022★ 17 cited

Backtracing the internal rotation history of the Cep star HD 129929

Sébastien Salmon, Facundo Moyano, Patrick Eggenberger +2

HD 129929 is a slowly-rotating Cephei pulsator with a rich spectrum of detected oscillations, including two rotational multiplets. The asteroseismic interpretation revealed the…

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.SR2022★ 48 cited

Trapping of HII regions in Population III star formation

Ondrej Jaura, Simon C. O. Glover, Katharina M. J. Wollenberg +3

Radiative feedback from massive Population III (Pop III) stars in the form of ionising and photodissociating photons is widely believed to play a central role in shutting off accre…

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…