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Binary Populations and Stellar Dynamics in Young Clusters

Published online by Cambridge University Press:  01 December 2007

D. Vanbeveren
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Brussels, Belgium email: [email protected], [email protected] GroupT, Association K.U. Leuven, Louvain, Belgium email: [email protected]
H. Belkus
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Brussels, Belgium email: [email protected], [email protected]
J. Van Bever
Affiliation:
Institute of Computational Astrophysics, St.-Mary's University, Halifax, Canada email: [email protected]
N. Mennekens
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Brussels, Belgium email: [email protected], [email protected]
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

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