A coupled galaxy-cluster model shows that Milky Way globular clusters, many from satellite galaxies, form dynamically interacting black hole binaries whose merger rates increase with redshift up to z=5.
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Chemo-dynamical study of eight UBC open clusters finds nearly circular thin-disk orbits with modest radial displacements under 0.5 kpc, indicating mild radial redistribution.
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Milky Way Globular Clusters: Nurseries for Dynamically-Formed Binary Black Holes
A coupled galaxy-cluster model shows that Milky Way globular clusters, many from satellite galaxies, form dynamically interacting black hole binaries whose merger rates increase with redshift up to z=5.
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Chemo-dynamical Analysis of Eight UBC Open Clusters
Chemo-dynamical study of eight UBC open clusters finds nearly circular thin-disk orbits with modest radial displacements under 0.5 kpc, indicating mild radial redistribution.