Intermediate-mass black holes in globular cluster systems

J. M. Wrobel, J. C.A. Miller-Jones, K. E. Nyland, T. J. Maccarone

Research output: Contribution to journalArticlepeer-review

Abstract

Using the Next Generation Very Large Array (ngVLA), we will make a comprehensive inventory of intermediate-mass black holes (IMBHs) in hundreds of globular cluster systems out to a distance of 25 Mpc. IMBHs have masses MIMBH ∼ 100 − 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. Reaching a large number of globular clusters is key, as Fragione et al. (2018) predict that only a few percent will have retained their gravitational-wave fostering IMBHs.

Original languageEnglish
JournalUnknown Journal
StatePublished - Jun 15 2018

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