Semianalytical Fokker–Planck Models for Nuclear Star Clusters

Semianalytical Fokker–Planck Models for Nuclear Star Clusters

We study the dynamics of nuclear star clusters, the dense stellar environments surrounding massive black holes in the centers of galaxies. We consider angular momentum diffusion due to two-body scatterings among stellar objects and energy advection due to gravitational-wave emission upon interaction...

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Bibliographic Details
Main Authors:	Karamveer Kaur, Barak Rom, Re’em Sari
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Series:	The Astrophysical Journal
Subjects:	Galaxy nuclei Stellar dynamics Supermassive black holes Stellar mass black holes Gravitational wave sources X-ray transient sources
Online Access:	https://doi.org/10.3847/1538-4357/ada8a8
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