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Intermediate-Mass Black Holes in Extragalactic Globular Clusters

Published onMay 31, 2019
Intermediate-Mass Black Holes in Extragalactic Globular Clusters
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Abstract

Intermediate-mass black holes have masses of ~100 to 100,000 M. Finding them in globular clusters would validate a formation channel for seed black holes in the early universe and inform event predictions for gravitational wave facilities. Searching many globular clusters is key, and only feasible using a next-generation Very Large Array.

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