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The multiplicity of massive stars: a 2016 view

Published online by Cambridge University Press:  28 July 2017

Hugues Sana
Hugues Sana*
Affiliation:
Institute of Astrophysics, KU Leuven, Celestijnlaan 200D, 3001 Leuven, Belgium email: [email protected]
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Abstract

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Massive stars like company. Here, we provide a brief overview of progresses made over the last 5 years by a number of medium and large surveys. These results provide new insights on the observed and intrinsic multiplicity properties of main sequence massive stars and on the initial conditions for their future evolution. They also bring new interesting constraints on the outcome of the massive star formation process.

Keywords

stars: early-typebinaries (including multiple): closebinaries: spectroscopicstars: individual (VFTS352, RMC145)binaries: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 110 - 117
Copyright
Copyright © International Astronomical Union 2017 

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