No radio emission was detected from X-ray-bright young massive cluster candidates in M51, placing an upper limit on accreting intermediate-mass black holes above roughly 10^4 solar masses.
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Detecting the Black Hole Candidate Population in M51's Young Massive Star Clusters: Constraints on Accreting Intermediate Mass Black Holes
No radio emission was detected from X-ray-bright young massive cluster candidates in M51, placing an upper limit on accreting intermediate-mass black holes above roughly 10^4 solar masses.