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The role of three-body stability in tidally interacting globular clusters

Published online by Cambridge University Press:  07 March 2016

Gareth F. Kennedy
Gareth F. Kennedy*
Affiliation:
National Astronomical Observatories of China, Chinese Academy of Sciences, Beijing 100012, China email: gareth.f.kennedy@gmail.com Monash Centre for Astrophysics, Monash University, Clayton, Vic, Australia, 3800
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Abstract

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The role of stability in the general three-body problem is investigated with regard to the tidal radius of a globular cluster (GC) in a galactic potential. This proceedings is a summary of two papers which outline the stability method (Kennedy 2014a) and compare the predicted stability boundary radius to observations of velocity dispersion profiles in Milky Way GCs (Kennedy 2014b).

Keywords

gravitationstellar dynamicsmethods: analyticalstars: kinematicsglobular clusters: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S312: Star Clusters and Black Holes in Galaxies across Cosmic Time , August 2014 , pp. 231 - 234
Copyright
Copyright © International Astronomical Union 2016 

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