Radio emission from the possible intermediate mass black hole in NGC 6388

Details Radio emission from the possible intermediate mass black hole in NGC 6388 Radio emission from the possible intermediate mass black hole in NGC 6388

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1657k&link_type=abstract

ATNF proposal C1793, Semester: October, 2008

Physics

Galactic, Atca

Scientific paper

Demonstration of the existence of intermediate mass black holes, with masses in the 100-10,000 solar mass range, would be of significant interest and could have implications for our understanding of the process of supermassive black hole formation, the dynamics of stellar clusters, and the physical nature of the ultraluminous X-ray sources. Recently, Lanzoni et al. (2007) reported evidence for an intermediate mass black hole in the globular cluster NGC 6388. If present, the object should produce radio emission. We propose to search for the predicted radio emission using ATCA.

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