Rapid formation of a very massive star (>50000 M⊙), and subsequently, of an IMBH, from runaway collisions Direct N-body and Monte Carlo simulations of dense star clusters
Year: 2026
Type: article
Source: MPG.PuRe (Max Planck Society)
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: closed
OpenAlex ID: W7128656042
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