activity
20022026
most citedGravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

612 citations · 5k across the 113 of their papers we have counts for

collaborators
Showing 2016Show all

5 papers · 1 filter

astro-ph.SR2016★ 15 cited

Analysis of the linear approximation of seismic inversions for various structural pairs

G. Buldgen, D. R. Reese, M. A. Dupret

Thanks to space-based photometry missions CoRoT and Kepler, we benefit from a wealth of seismic data for stars other than the sun. In the future, K2, Tess, and Plato will complemen…

astro-ph.SR2016★ 25 cited

Apsidal motion in the massive binary HD152218

G. Rauw, S. Rosu, A. Noels +5

Massive binary systems are important laboratories in which to probe the properties of massive stars and stellar physics in general. In this context, we analysed optical spectroscop…

astro-ph.SR2016★ 33 cited

In-depth study of 16CygB using inversion techniques

G. Buldgen, S. J. A. S. Salmon, D. R. Reese +1

The 16Cyg binary system hosts the solar-like Kepler targets with the most stringent observational constraints. Moreover, this system is particularly interesting since both stars ar…

astro-ph.SR2016★ 15 cited

The IACOB project: IV. New predictions for high-degree non-radial mode instability domains in massive stars and connection with macroturbulent broadening

M. Godart, S. Simón-Díaz, A. Herrero +4

Asteroseismology is a powerful tool to access the internal structure of stars. Apart from the important impact of theoretical developments, progress in this field has been commonly…

astro-ph.SR2016★ 77 cited

Interaction Between Convection and Pulsation

Günter Houdek, Marc-Antoine Dupret

This article reviews our current understanding of modelling convection dynamics in stars. Several semi-analytical time-dependent convection models have been proposed for pulsating…