activity
20082013
most citedCommon Envelope Evolution: Where we stand and how we can move forward

1k citations · 1.2k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2013★ 7 cited

A two-dimensional mixing length theory of convective transport

P. Lesaffre, S. M. Chitre, A. T. Potter +1

The helioseismic observations of the internal rotation profile of the Sun raise questions about the two-dimensional (2D) nature of the transport of angular momentum in stars. Here…

astro-ph.HE2012★ 1k cited

Common Envelope Evolution: Where we stand and how we can move forward

N. Ivanova, S. Justham, X. Chen +16

This work aims to present our current best physical understanding of common-envelope evolution (CEE). We highlight areas of consensus and disagreement, and stress ideas which shoul…

astro-ph.SR2012★ 1 cited

Rotation and Magnetism in Massive Stars

Adrian T. Potter

Rotation has a number of important effects on the evolution of stars. It decreases the surface gravity, causes enhanced mass loss and leads to surface abundance anomalies of variou…

astro-ph.SR2012★ 45 cited

Stellar evolution of massive stars with a radiative alpha-omega dynamo

Adrian T. Potter, Shashikumar M. Chitre, Christopher A. Tout

Models of rotationally-driven dynamos in stellar radiative zones have suggested that magnetohydrodynamic transport of angular momentum and chemical composition can dominate over th…

astro-ph.SR2012★ 20 cited

Towards a unified model of stellar rotation II: Model-dependent characteristics of stellar populations

Adrian T. Potter, Christopher A. Tout, Ines Brott

Rotation has a number of important effects on the evolution of stars. Apart from structural changes because of the centrifugal force, turbulent mixing and meridional circulation ca…

astro-ph.SR2011★ 37 cited

Towards a unified model of stellar rotation

Adrian T. Potter, Christopher A. Tout, John J. Eldridge

The effects of rapid rotation on stellar evolution can be profound. We are now beginning to gather enough data to allow a realistic comparison between different physical models. Tw…