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20152026
most citedMerging black holes in young star clusters

271 citations · 764 across the 11 of their papers we have counts for

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA2026

Constraining the Galactic bar and spiral pattern speeds with the Hyades tidal stream

Zi-yi Zhou, Long Wang, Tereza Jerabkova +1

We present a suite of direct -body simulations of the Hyades open cluster and its tidal stream in a Milky Way potential that includes a rotating bar and spiral arms. Using the h…

astro-ph.GA2021

SIRIUS Project. III. Star-by-star simulations of star cluster formation using a direct N-body integrator with stellar feedback

Michiko S. Fujii, Takayuki R. Saitoh, Yutaka Hirai +1

One of the computational challenges of cluster formation simulations is resolving individual stars and simulating massive clusters with masses of more than without…

astro-ph.GA2021

SIRIUS project II: a new tree-direct hybrid code for smoothed particle hydrodynamics/N-body simulations of star clusters

M. S. Fujii, T. R. Saitoh, L. Wang +1

Star clusters form via clustering star formation inside molecular clouds. In order to understand the dynamical evolution of star clusters in their early phase, in which star cluste…

astro-ph.GA2020

Intermediate Mass Black Hole Formation in compact Young Massive Star Clusters

Francesco Paolo Rizzuto, Thorsten Naab, Rainer Spurzem +6

Young dense massive star clusters are a promising environment for the formation of intermediate mass black holes (IMBHs) through collisions. We present a set of 80 simulations carr…

astro-ph.GA2020123 cited

Very high redshift quasars and the rapid emergence of super-massive black holes

Pavel Kroupa, Ladislav Subr, Tereza Jerabkova +1

The observation of quasars at very high redshift such as Poniuaena is a challenge for models of super-massive black hole (SMBH) formation. This work presents a study of SMBH format…

astro-ph.GA201928 cited

The survival of star clusters with black hole subsystems

Long Wang

Recent observations have detected top-heavy IMFs in dense star forming regions like the Arches cluster. Whether such IMFs also exist in old dense stellar systems like globular clus…