THE ABSENCE OF RADIO EMISSION FROM THE GLOBULAR CLUSTER G1
THE ABSENCE OF RADIO EMISSION FROM THE GLOBULAR CLUSTER G1
The detections of both X-ray and radio emission from the cluster G1 in M31 have provided strong support for existing dynamical evidence for an intermediate mass black hole (IMBH) of mass 1.8 +/- 0.5 x 10^4 solar masses at the cluster center. However, given the relatively low significance and astrometric …