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19962009
most citedA Dynamical Model for the Globular Cluster G1

166 citations · 514 across the 7 of their papers we have counts for

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astro-ph2008★ 37 cited

Trojan Stars in the Galactic Center

Michiko Fujii, Masaki Iwasawa, Yoko Funato +1

We performed, for the first time, the simulation of spiral-in of a star cluster formed close to the Galactic center (GC) using a fully self-consistent -body model. In our model,…

astro-ph2006★ 29 cited

The core radius of a star cluster containing a massive black hole

Douglas C. Heggie, Piet Hut, Shin Mineshige +2

(Simplified) We present a theoretical framework which establishes how the core radius of a star cluster varies with the mass of an assumed central black hole. Our result is that th…

astro-ph2005★ 55 cited

Tidal Capture of Stars by Intermediate-Mass Black Holes

H. Baumgardt, C. Hopman, S. Portegies Zwart +1

Recent X-ray observations and theoretical modelling have made it plausible that some ultraluminous X-ray sources (ULX) are powered by intermediate-mass black holes (IMBHs). N-body…

astro-ph2003★ 166 cited

A Dynamical Model for the Globular Cluster G1

Holger Baumgardt, Junichiro Makino, Piet Hut +2

We present a comparison between the observational data on the kinematical structure of G1 in M31, obtained with the Hubble WFPC2 and STIS instruments, and the results of dynamical…

astro-ph1996★ 97 cited

Evolution of Compact Groups of Galaxies I. Merging Rates

E. Athanassoula, J. Makino, A. Bosma

We discuss the merging rates in compact groups of 5 identical elliptical galaxies. All groups have the same mass and binding energy. We consider both cases with individual halos an…

astro-ph1996★ 40 cited

Time-Symmetrized Kustaanheimo-Stiefel Regularization

Y. Funato, P. Hut, S. McMillan +1

In this paper we describe a new algorithm for the long-term numerical integration of the two-body problem, in which two particles interact under a Newtonian gravitational potential…