199 citations · 673 across the 9 of their papers we have counts for
8 papers · 1 filter
The magneto-rotational instability in massive stars
A. Griffiths, G. Meynet, P. Eggenberger +2
The interaction between weak magnetic fields and rotation can lead to instabilities that transport angular momentum (AM) and chemical elements affecting the evolution of massive st…
Stellar variability in open clusters. II. Discovery of a new period-luminosity relation in a class of fast-rotating pulsating stars in NGC 3766
N. Mowlavi, S. Saesen, T. Semaan +5
Pulsating stars are windows to the physics of stars enabling us to see glimpses of their interior. Not all stars pulsate, however. On the main sequence, pulsating stars…
Massive star evolution in close binaries:conditions for homogeneous chemical evolution
H. F. Song, G. Meynet, A. Maeder +2
We investigate the impact of tidal interactions, before any mass transfer, on various properties of the stellar models. We study the conditions for obtaining homogeneous evolution…
Prospects for asteroseismic inference on the envelope helium abundance in red giant stars
A. -M. Broomhall, A. Miglio, J. Montalban +6
Regions of rapid variation in the internal structure of a star are often referred to as acoustic glitches since they create a characteristic periodic signature in the frequencies o…
Star formation with disc accretion and rotation I. Stars between 2 and 22 Msol at solar metallicity
L. Haemmerlé, P. Eggenberger, G. Meynet +2
The way angular momentum is built up in stars during their formation process may have an impact on their further evolution. In the frame of the cold disc accretion scenario, we stu…
Populations of rotating stars. - I. Models from 1.7 to 15 Msun at Z = 0.014, 0.006, and 0.002 with Ω/Ωcrit between 0 and 1
Cyril Georgy, Sylvia Ekström, Anahí Granada +4
B-type stars are known to rotate at various velocities, including very fast rotators near the critical velocity as the Be stars. In this paper, we provide stellar models covering t…