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Binary Populations and Stellar Dynamics in Young Clusters

Published online by Cambridge University Press:  01 December 2007

D. Vanbeveren ,
H. Belkus ,
J. Van Bever  and
N. Mennekens
D. Vanbeveren
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Brussels, Belgium email: dvbevere@vub.ac.be, hbelkus@vub.ac.be GroupT, Association K.U. Leuven, Louvain, Belgium email: dany.vanbeveren@groept.be
H. Belkus
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Brussels, Belgium email: dvbevere@vub.ac.be, hbelkus@vub.ac.be
J. Van Bever
Affiliation:
Institute of Computational Astrophysics, St.-Mary's University, Halifax, Canada email: vanbever@penguin.stmarys.ca
N. Mennekens
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Brussels, Belgium email: dvbevere@vub.ac.be, hbelkus@vub.ac.be
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Abstract

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We first summarize work that has been done on the effects of binaries on theoretical population synthesis of stars and stellar phenomena. Next, we highlight the influence of stellar dynamics in young clusters by discussing a few candidate UFOs (unconventionally formed objects) like intermediate mass black holes, η Car, ζ Pup, γ2 Velorum and WR 140.

Keywords

binaries: close – Galaxy: kinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S250: Massive Stars as Cosmic Engines , December 2007 , pp. 293 - 300
Copyright
Copyright © International Astronomical Union 2008

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