Growth of A Massive Black Hole Via Tidal Disruption Accretion

Stars that are tidally disrupted by the massive black hole (MBH) may contribute significantly to the growth of the MBH, especially in dense nuclear star clusters (NSCs). Yet, this tidal disruption accretion (TDA) of stars onto the MBH has largely been overlooked compared to the gas accretion (GA) ch...

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Veröffentlicht in:	arXiv.org 2022-11
Hauptverfasser:	Lee, Seungjae, Ji-hoon, Kim, Oh, Boon Kiat
Format:	Artikel
Sprache:	eng
Schlagworte:	Deposition Disruption Evolution Finite element method Grid refinement (mathematics) Physics - Astrophysics of Galaxies Star & galaxy formation Star clusters Star formation Supermassive black holes
Online-Zugang:	Volltext
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