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) × 10^4 M ? at the cluster center. However, given the relatively low significance and astrometric accu...

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Bibliographic Details
Main Authors: Miller-Jones, James, Wrobel, J., Sivakoff, G., Heinke, C., Miller, R., Plotkin, R., Di Stefano, R., Greene, J., Ho, L., Joseph, T., Kong, A., Maccarone, T.
Format: Journal Article
Published: Institute of Physics Publishing Ltd. 2012
Subjects:
accretion
accretion disks
globular clusters: individual (Mayall-II = G1)
X-rays: binaries
Online Access:http://hdl.handle.net/20.500.11937/20357

Internet

http://hdl.handle.net/20.500.11937/20357

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