103 citations · 812 across the 62 of their papers we have counts for
9 papers · 1 filter
Asteroseismology of Cephei stars: The stellar inferences tested in hare and hound exercises
Sébastien Salmon, Patrick Eggenberger, Josefina Montalbán +5
The Cephei pulsators are massive main-sequence stars, presenting low radial-order modes. These modes probe in particular the chemical gradient at the edge of the convective cor…
Kepler-93: a testbed for detailed seismic modelling and orbital evolution of super-earths around solar-like stars
J. Bétrisey, C. Pezzotti, G. Buldgen +4
The advent of space-based photometry missions such as CoRoT, Kepler and TESS has sparkled the development of asteroseismology and exoplanetology. The advent of PLATO will further s…
The key impact of the host star's rotational history on the evolution of TOI-849b
C. Pezzotti, O. Attia, P. Eggenberger +2
TOI-849b is one of the few planets populating the hot-Neptune desert and it is the densest Neptune-sized one discovered so far. Its extraordinary proximity to the host star, togeth…
Asteroseismology of evolved stars to constrain the internal transport of angular momentum. IV. Internal rotation of Kepler 56 from an MCMC analysis of the rotational splittings
L. Fellay, G. Buldgen, P. Eggenberger +4
The observations of global stellar oscillations of post main-sequence stars by space-based photometry missions allowed to directly determine their internal rotation. These constrai…
Standard solar models: a perspective from updated solar neutrino fluxes and the gravity-mode period spacing
Sébastien Salmon, Gaël Buldgen, Arlette Noels +3
Context: The Sun is by far a privileged target for testing stellar models with unique precision. A recent concern appeared with the progress in the solar surface abundances derivat…
Star-planet interactions VI. Tides, stellar activity and planet evaporation
Suvrat Rao, Camilla Pezzotti, Georges Meynet +6
Tidal interactions and planet evaporation processes impact the evolution of close-in star-planet systems. We study the impact of stellar rotation on these processes. We compute the…