SUPER MASSIVE BLACK HOLE IN GALACTIC NUCLEI WITH TIDAL DISRUPTION OF STARS

Tidal disruption of stars by super massive central black holes from dense star clusters is modeled by high-accuracy direct N-body simulation. The time evolution of the stellar tidal disruption rate, the effect of tidal disruption on the stellar density profile, and, for the first time, the detailed...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	The Astrophysical journal 2014-09, Vol.792 (2), p.137
Hauptverfasser:	Zhong, Shiyan, Berczik, Peter, Spurzem, Rainer
Format:	Artikel
Sprache:	eng
Schlagworte:	ACCURACY ANISOTROPY ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BLACK HOLES COMPARATIVE EVALUATIONS COMPUTERIZED SIMULATION DENSITY EVOLUTION GALAXIES GALAXY NUCLEI ORBITS QUASARS STAR CLUSTERS STARS VELOCITY
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!