The Gravitational Million-Body Problem: A Multidisciplinary Approach to Star Cluster Dynamics

By D Heggie, P Hut. 2003

147 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/d35c3988f2eb1069dd2ae0f044361df1d6aadbec

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. F. Rasio
2. S. Goswami
3. Matthew Bierbaum
4. S. Umbreit
5. S. Banerjee
6. F. Antonini
7. M. Volonteri
8. S. Naoz

In Statistical and Nonlinear Physics

1. S. Goswami
2. Matthew Bierbaum
3. S. Umbreit
4. F. Rasio

Citations in the corpus

• Stellar Dynamics and Stellar Phenomena Near a Massive Black Hole (2017, unknown): “The MBH’s mass scales with the bulge’s mass Mb as M• = •Mb, with • ∼ (1− 2)× 10−3 (Magorrian et al. 1998; Häring & Rix 2004).”
• Formation of Massive Black Holes in Dense Star Clusters. I. Mass Segregation and Core Collapse (2003, methodology): “Numerical methods for investigating the dynamical evolution of star clusters include direct N -body integration , solutions of the Fokker-Planck equation by direct (finite-difference) or Monte Carlo methods, and gaseous models (for a review, see Heggie & Hut 2003).”