142 citations · 567 across the 14 of their papers we have counts for
14 papers
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…
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…
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…
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…
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…
γ Doradus stars as test of angular momentum transport models
Rhita-Maria Ouazzani, J. P. Marques, M-J. Goupil +3
Helioseismology and asteroseismology of red giant stars have shown that the distribution of angular momentum in stellar interiors, and its evolution with time remains an open issue…
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…
A new asteroseismic diagnostic for internal rotation in Doradus stars
Rhita-Maria Ouazzani, S. J. A. J. Salmon, V. Antoci +3
With four years of nearly-continuous photometry from Kepler, we are finally in a good position to apply asteroseismology to Doradus stars. In particular several analyses have d…
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…
Are the stars of a new class of variability detected in NGC~3766 fast rotating SPB stars?
S. J. A. J. Salmon, J. Montalbán, D. R. Reese +2
A recent photometric survey in the NGC~3766 cluster led to the detection of stars presenting an unexpected variability. They lie in a region of the Hertzsprung-Russell (HR) diagram…
Asteroseismology of Massive Stars : Some Words of Caution
A. Noels, M. Godart, S. Salmon +3
Although playing a key role in the understanding of the supernova phenomenon, the evolution of massive stars still suffers from uncertainties in their structure, even during their…
Kepler observations of variability in B-type stars
L. A. Balona, A. Pigulski, P. De Cat +27
The analysis of the light curves of 48 B-type stars observed by Kepler is presented. Among these are 15 pulsating stars, all of which show low frequencies characteristic of SPB sta…
Can an underestimation of opacity explain B-type pulsators in the SMC?
S. Salmon, J. Montalbán, A. Miglio +3
Slowly Pulsating B and Cephei are mechanism driven pulsating B stars. That mechanism works since a peak in the opacity due to a high number of atomic transitions from i…
The Enigma of B-type Pulsators in the SMC
S. Salmon, J. Montalban, A. Miglio +3
Since the early nineties it is accepted that the excitation mechanism of B-type pulsators on the main sequence is due to the opacity peak in the iron-group elements at $T\approx 20…