activity
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

collaborators
Showing astro-ph.SRShow all

5 papers · 1 filter

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.SR2018★ 60 cited

Star-planet interactions. V. Dynamical and equilibrium tides in convective zones

Suvrat Rao, Georges Meynet, Patrick Eggenberger +5

When planets are formed from the protoplanetary disk and after the disk has dissipated, the evolution of their orbits is governed by tidal interactions, friction, and gravitational…

astro-ph.SR2015★ 45 cited

Massive star formation by accretion I. Disc accretion

Lionel Haemmerlé, Patrick Eggenberger, Georges Meynet +2

Massive stars likely form by accretion and the evolutionary track of an accreting forming star corresponds to what is called the birthline in the HR diagram. The shape of this birt…