most citedRotating massive stars: Pre-SN models and stellar yields at solar metallicity

10 citations · 11 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph200410 cited

Rotating massive stars: Pre-SN models and stellar yields at solar metallicity

R. Hirschi, G. Meynet, A. Maeder

We present a new set of stellar yields obtained from rotating stellar models at solar metallicity covering the massive star range (9-120 solar masses). The stellar models were calc…

astro-ph2004

Rotation and Mixing in Massive Stars: Principles and Uncertainties

Georges Meynet, Andre Maeder

The main instabilities induced by rotation in stellar interiors are described. We derive from first principles the general equation describing the transport of the angular momentum…

astro-ph2004

Chemical Abundances and Yields from Massive Stars

André Maeder, Georges Meynet, Raphael Hirschi

Stellar rotation produces an internal mixing of the elements due to shear instability and meridional circulation. This leads to observable enhancements in massive stars above…

astro-ph2004

Effects of Rotation on Presupernovae Models

Georges Meynet, Raphael Hirschi, André Maeder

We show that rotation strongly affects the nature of the supernova progenitor (blue/red supergiant or Wolf--Rayet star), and thus the supernova types. In particular our models well…

astro-ph2004

Evolution at very low and zero Z

Georges Meynet, André Maeder, Sylvia Ekström

Rotation deeply affects the evolution of very metal poor massive stars. Indeed, even moderately rotating stars reach the break--up limit during the Main--Sequence (MS) phase, they…

astro-ph20041 cited

Evolution of the Most Massive Stars

André Maeder, Georges Meynet, Raphael Hirschi

We discuss the physics of the -- Limit, i.e. when the star is unbound as a result of {\emph{both}} rotation and radiation pressure. We suggest that the -- Limit is what mak…