Georges Meynet, Andre Maeder, Patrick Eggenberger, Sylvia Ekstrom, Cyril Georgy, Cristina Chiappini, Giovanni Privitera, Arthur Choplin
Published 2015-12-02Version 1
After a brief recall of the main impacts of stellar rotation on the structure and the evolution of stars, four topics are addressed: 1) the links between magnetic fields and rotation; 2) the impact of rotation on the age determination of clusters; 3) the exchanges of angular momentum between the orbit of a planet and the star due to tides; 4) the impact of rotation on the early chemical evolution of the Milky Way and the origin of the Carbon-Enhanced-Metal-Poor stars.
Comments: 5 pages, 2 figures, To appear in Astronomische Nachrichten, special issue "Reconstruction the Milky Way's History: Spectroscopic surveys, Asteroseismology and Chemo-dynamical models", Guest Editors C. Chiappini, J. Montalban, and M. Steffen, AN 2016 (in press)
Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002
The First Two Thousand Years of Star Formation
How accurate are stellar ages based on stellar models? II. The impact of asteroseismology
![QR code for arXiv:1512.00767 [astro-ph.SR]](http://oss.arxitics.com/images/favicon.svg)