activity
20142026
most citedChronologically dating the early assembly of the Milky Way

129 citations · 1.4k across the 81 of their papers we have counts for

collaborators
Showing 2023Show all

6 papers · 1 filter

astro-ph.SR2023

Asteroseismic modelling strategies in the PLATO era. II. Automation of seismic inversions and quality assessment procedure

Jérôme Bétrisey, Gaël Buldgen, Daniel R. Reese +1

*Context*. In the framework of the PLATO mission, to be launched in late 2026, seismic inversion techniques will play a key role in the mission precision requirements of the stella…

astro-ph.SR2023★ 1 cited

The evolution and impact of 3000 M stars in the early Universe

D. Nandal, E. Farrell, G. Buldgen +2

We present evolutionary models of massive, accreting population III stars with constant and variable accretion rates until the end of silicon burning, with final masses of 1000 - 3…

astro-ph.SR2023

Helioseismic determination of the solar metal mass fraction

G. Buldgen, A. Noels, V. A. Baturin +5

Context. The metal mass fraction of the Sun Z is a key constraint in solar modelling, but its value is still under debate. The standard solar chemical composition of the late 2000s…

astro-ph.SR2023★ 11 cited

Asteroseismic modelling strategies in the PLATO era I. Mean density inversions and direct treatment of the seismic information

Jérôme Bétrisey, Gaël Buldgen, Daniel R. Reese +6

Asteroseismic modelling will be part of the pipeline of the PLATO mission and will play a key role in the mission precision requirements on stellar mass, radius and age. It is ther…

astro-ph.SR2023★ 19 cited

Testing angular momentum transport processes with asteroseismology of solar-type main-sequence stars

Jérôme Bétrisey, Patrick Eggenberger, Gaël Buldgen +2

Asteroseismology has become a powerful tool to study the internal rotation of stars, and its study allows to constrain the internal AM transport processes and better understand the…

astro-ph.SR2023★ 9 cited

Glitches in solar-like oscillating F-type stars: Theoretical signature of the base of the convective envelope on the ratios

M. Deal, M. -J. Goupil, M. S. Cunha +7

The transition between convective and radiative stellar regions is still not fully understood. The sharp variations in sound speed located in these transition regions give rise to…