Rapid formation of a very massive star >50000 $M_\odot$ and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters

Fuente: arXiv

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Bibliographic Details
Main Authors:	Vergara, Marcelo C., Askar, Abbas, Kamlah, Albrecht W. H., Spurzem, Rainer, Dotti, Francesco Flammini, Schleicher, Dominik R. G., Sedda, Manuel Arca, Hypki, Arkadiusz, Giersz, Mirek, Hurley, Jarrod, Berczik, Peter, Escala, Andres, Hoyer, Nils, Neumayer, Nadine, Pang, Xiaoying, Tanikawa, Ataru, Cen, Renyue, Naab, Thorsten
Format:	Preprint
Published:	2025
Subjects:	Astrophysics of Galaxies High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2505.07491