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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A model where maximum cluster mass scales with star formation rate explains the LMC age gap as resulting from low-SFR periods producing only faint clusters that are now hard to detect.
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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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The apparent Large Magellanic Cloud star cluster age gap
A model where maximum cluster mass scales with star formation rate explains the LMC age gap as resulting from low-SFR periods producing only faint clusters that are now hard to detect.