activity
20192023
most citedTwo-dimensional simulations of internal gravity waves in a 5 Zero-Age-Main-Sequence model

14 citations · 25 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.SR20242 cited

Effects of stratification on overshooting and waves atop the convective core of main-sequence stars

Adrien Morison, Arthur Le Saux, Isabelle Baraffe +5

As a massive star evolves along the main sequence, its core contracts, leaving behind a stable stratification in helium. We simulate 2D convection in the core at three different st…

astro-ph.SR202314 cited

Two-dimensional simulations of internal gravity waves in a 5 Zero-Age-Main-Sequence model

A. Le Saux, I. Baraffe, T. Guillet +5

Main-sequence intermediate-mass stars present a radiative envelope that supports internal gravity waves (IGWs). Excited at the boundary with the convective core, IGWs propagate tow…

astro-ph.SR20228 cited

Local heating due to convective overshooting and the solar modelling problem

Baraffe I, Constantino T, Clarke J +5

Recent hydrodynamical simulations of convection in a solar-like model suggest that penetrative convective flows at the boundary of the convective envelope modify the thermal backgr…

astro-ph.SR20191 cited

Automatic classification of K2 pulsating stars using machine learning techniques

A. Le Saux, L. Bugnet, S. Mathur +2

The second mission of the NASA Kepler satellite, K2, has collected hundreds of thousands of lightcurves for stars close to the ecliptic plane. This new sample could increase the nu…

astro-ph.SR20192 cited

Determining surface rotation periods of solar-like stars observed by the Kepler mission using machine learning techniques

S. N. Breton, L. Bugnet, A. R. G. Santos +4

For a solar-like star, the surface rotation evolves with time, allowing in principle to estimate the age of a star from its surface rotation period. Here we are interested in measu…