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Rotation and Massive Close Binary Evolution

Published online by Cambridge University Press:  01 December 2007

Norbert Langer ,
Matteo Cantiello ,
Sung-Chul Yoon ,
Ian Hunter ,
Ines Brott ,
Danny Lennon ,
Selma de Mink  and
Marcel Verheijdt
Norbert Langer
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
Matteo Cantiello
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
Sung-Chul Yoon
Affiliation:
University of California, Santa Cruz, USA
Ian Hunter
Affiliation:
The Queen's University of Belfast, Northern Ireland, UK
Ines Brott
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
Danny Lennon
Affiliation:
Isaac Newton Group, Santa Cruz de La Palma, Canary Islands, Spain
Selma de Mink
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
Marcel Verheijdt
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
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Abstract

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We review the role of rotation in massive close binary systems. Rotation has been advocated as an essential ingredient in massive single star models. However, rotation clearly is most important in massive binaries where one star accretes matter from a close companion, as the resulting spin-up drives the accretor towards critical rotation. Here, we explore our understanding of this process, and its observable consequences. When accounting for these consequences, the question remains whether rotational effects in massive single stars are still needed to explain the observations.

Keywords

stars: early-type – stars: fundamental parameters – stars: mass loss – stars: rotation – stars: binaries: close
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S250: Massive Stars as Cosmic Engines , December 2007 , pp. 167 - 178
Copyright
Copyright © International Astronomical Union 2008

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