Hybrid hydro/direct N-body simulations of dense high-redshift gas clouds form very massive stars via runaway collisions that collapse to IMBHs capable of growing from ~6700 to ~62000 solar masses in 100 Myr under optimistic assumptions.
Spatially Resolved Physical Properties of Young Star Clusters and Star-forming Clumps in the Brightest z¿6 Galaxy, the Strongly Lensed Cosmic Spear at z=6.2
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