88 citations · 165 across the 6 of their papers we have counts for
6 papers
Constraining the efficiency of angular momentum transport with asteroseismology of red giants: the effect of stellar mass
P. Eggenberger, N. Lagarde, A. Miglio +12
Context: Constraints on the internal rotation of red giants are now available thanks to asteroseismic observations. Preliminary comparisons with rotating stellar models indicate th…
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…
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…
The puzzling new class of variable stars in NGC 3766 : old friend pulsators?
S. J. A. J. Salmon, J. Montalbàn, D. R. Reese +2
The recent variability survey of the NGC 3766 cluster revealed a considerable number of periodic variable stars in a region of the H-R diagram where no pulsation is expected. This…
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…