activity
20172020
most citedFirst evidence of inertial modes in Doradus stars: The core rotation revealed

64 citations · 85 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.SR202064 cited

First evidence of inertial modes in Doradus stars: The core rotation revealed

R-M. Ouazzani, F. Lignières, M-A. Dupret +4

Gamma Doradus stars present an incredibly rich pulsation spectra, with gravito-inertial modes, in some cases supplemented with delta Scuti-like pressure modes and in numerous cases…

astro-ph.SR2020

The prototype star Doradus observed by TESS

S. Christophe, V. Antoci, E. Brunsden +2

Doradus is the prototype star for the eponymous class of pulsating stars that consists of late A-early F main-sequence stars oscillating in low-frequency gravito-inertial modes…

astro-ph.SR201820 cited

Comprehensive stellar seismic analysis : New method exploiting the glitches information in solar-like pulsators

M. Farnir, M-A. Dupret, S. J. A. J. Salmon +2

Aims: We develop a method that provides a comprehensive analysis of the oscillation spectra of solar-like pulsators. We define new seismic indicators that should be as uncorrelated…

astro-ph.SR2018

The asteroseismic potential of CHEOPS

A. Moya, S. Barceló Forteza, A. Bonfanti +3

Asteroseismology has been impressively boosted during the last decade mainly thanks to space missions such as Kepler/K2 and CoRoT. This has a large impact, in particular, in exopla…

astro-ph.SR2018

Deciphering the oscillation spectrum of Doradus and SPB stars

S. Christophe, J. Ballot, R. -M. Ouazzani +2

The space-based Kepler mission provided four years of highly precise and almost uninterrupted photometry for hundreds of Doradus stars and tens of SPB stars, finally allowing u…

astro-ph.SR20171 cited

The γ Dor stars as revealed by Kepler : A key to reveal deep-layer rotation in A and F stars

S. J. A. J. Salmon, R. -M. Ouazzani, V. Antoci +2

The γ Dor pulsating stars present high-order gravity modes, which make them important targets in the intermediate-and low-mass main-sequence region of the Hertzsprung-Russell diagr…