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The Chandrasekhar Spitzer controversy and the (ir)relevance of distant interactions

Published online by Cambridge University Press:  11 March 2020

Tjeerd S. van Albada
Affiliation:
Kapteyn Astronomical Institute, P.O. Box 800, 9700AVGroningen, the Netherlands email: [email protected]
Arpad Szomoru
Affiliation:
Joint Institute for VLBI ERIC, Oude Hoogeveensedijk 4, 7991PDDwingeloo, the Netherlands email: [email protected]
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Abstract

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We have done N-body simulations with N up to 106, with the aim to determine whether fluctuations in the force field of a globular cluster are caused by nearby or distant encounters. We find that distant encounters are insignificant, in agreement with Chandrasekhar’s expectations, contrary to general opinion.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

Binney, J. & Tremaine, S. 2008, Galactic Dynamics (Princeton University Press)CrossRefGoogle Scholar
Chandrasekhar, S. 1942, Principles of Stellar Dynamics (Dover Publications, Inc.)Google Scholar
Hénon, M. 1960, Ann. d’Aph., 23, 668Google Scholar
Huang, S., Dubinski, J., & Carlberg, R. G. 1993, ApJ, 404, 73CrossRefGoogle Scholar
Kandrup, H. E. 1980, Physics Reports 63, 1CrossRefGoogle Scholar
McMillan, S., Casertano, S., & Hut, P. 1988, in The Few Body Problem, IAU Coll. 96, 313CrossRefGoogle Scholar
Spitzer, L. 1987, Dynamical Evolution of Globular Clusters (Princeton University Press)Google Scholar
Theuns, T. 1996, MNRAS 279, 827CrossRefGoogle Scholar
Woltjer, L. 1967, Relativity Theory and Astrophysics, 2. Galactic Structure p. 1Google Scholar