Star Cluster Collapse and Massive Black Hole

Details Star Cluster Collapse and Massive Black Hole Star Cluster Collapse and Massive Black Hole

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.1654n&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

A cluster of compact objects (neutron stars and/or black holes) may mimic the presence of a super-massive black hole (SBH) at the center of the Galaxy. The cluster, with eventually a less massive black hole at its center, could be the remnant of a more massive cluster which has lost part of its mass. We use simple dynamical considerations to derive a lower limit to the mass of the black hole at the cluster center.

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