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Tidal Stripping and Disruption of Globular Clusters

Published online by Cambridge University Press:  04 August 2017

T.S. van Albada  and
T. R. Bontekoe
T.S. van Albada
Affiliation:
Kapteyn Astronomical Institute Postbus 800 9700 AV Groningen
T. R. Bontekoe
Affiliation:
Kapteyn Astronomical Institute Postbus 800 9700 AV Groningen

Extract

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Tidal stripping and disruption of globular clusters may be responsible for the absence of low density clusters in the inner region of the Galaxy. We have studied these processes by integrating orbits of stars while the cluster is moving through a spherically symmetric galactic potential with constant circular velocity (Vcir =220 km/s). The response of the cluster to the tidal field of the galaxy is calculated in a selfconsistent manner with a collisionless N-body code with N=5000 (van Albada 1982, van Albada and Bontekoe in preparation).

Type
May 31: External Fields and Finite-Star-Size Effects
Information
Symposium - International Astronomical Union , Volume 113: Dynamic of Stars Clusters , 1985 , pp. 423 - 425
Copyright
Copyright © Reidel 1985 

References

Fall, S.M. and Rees, M.J., 1977, M.N.R.A.S., 181 37P.Google Scholar
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van Albada, T.S., 1982, M.N.R.A.S., 201, 939.CrossRefGoogle Scholar
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