$Gravitational collapse at low to moderate Mach numbers: The relationship between star formation efficiency and the fraction of mass in the massive object$

Gravitational collapse at low to moderate Mach numbers: The relationship between star formation efficiency and the fraction of mass in the massive object

The formation of massive objects via gravitational collapse is relevant both for explaining the origin of the first supermassive black holes and in the context of massive star formation. Here, we analyze simulations of the formation of massive objects pursued by different groups and in various envir...

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Veröffentlicht in:	arXiv.org 2024-08
Hauptverfasser:	Saavedra-Bastidas, Jorge, Schleicher, Dominik R G, Klessen, Ralf S, Chon, Sunmyon, Omukai, Kazuyuki, Peters, Thomas, Prole, Lewis R, Reinoso, Bastián, Riaz, Rafeel, Solar, Paulo
Format:	Artikel
Sprache:	eng
Schlagworte:	Collision parameters Dimensionless analysis Efficiency Gravitational collapse Mach number Machine learning Massive stars Parameter estimation Physics - Astrophysics of Galaxies Protostars Simulation Slopes Star & galaxy formation Star formation Statistical correlation Stellar mass Supermassive black holes
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