activity
19952011
most citedThe Effective Temperatures and Physical Properties of Magellanic Cloud Red Supergiants: The Effects of Metallicity

219 citations · 919 across the 29 of their papers we have counts for

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Showing 2005Show all

6 papers · 1 filter

astro-ph2005

Evolution of rotating stars at very low metallicity

Georges Meynet, Raphael Hirschi, Sylvia Ekstrom +1

At very low metallicity, the effects of differential rotation have a more important impact on the evolution of stars than at high metallicity. Rotational mixing leads to the produc…

astro-ph2005

Single massive stars at the critical rotational velocity: possible links with Be and B[e] stars

Georges Meynet, Andre Maeder

Using single star models including the effects of shellular rotation with and without magnetic fields, we show that massive stars at solar metallicity with initial masses lower tha…

astro-ph2005

Effects of Rotation on Mass Loss for Population III stars

Sylvia Ekström, Georges Meynet, André Maeder

The effects of rotation on low-metallicity stellar models are twofold: first, the models reach break-up during main sequence and may lose mass by mechanical process; second, strong…

astro-ph2005

Evolution of the First Stars: CNO Yields and the C-rich Extremely Metal Poor Stars

Georges Meynet, Sylvia Ekstrom, Andre Maeder

Rotating massive stars at and lose a great part of their initial mass through stellar winds. The chemical composition of the rotationally enhanced winds of ve…

astro-ph2005

Stellar Evolution with Rotation and Magnetic Fields IV: The Solar Rotation Profile

P. Eggenberger, A. Maeder, G. Meynet

We examine the generation of a magnetic field in a solar-like star and its effects on the internal distribution of the angular velocity. We suggest that the evolution of a rotating…

astro-ph2005

Stellar evolution with rotation and magnetic fields:III: The interplay of circulation and dynamo

André Maeder, Georges Meynet

We examine the effects of the magnetic field created by the Tayler--Spruit dynamo in differentially rotating stars. Magnetic fields of the order of a few G are present throu…