Intermediate Mass Black Holes in Galactic Globular Clusters

Details Intermediate Mass Black Holes in Galactic Globular Clusters Intermediate Mass Black Holes in Galactic Globular Clusters

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1240..245j&link_type=abstract

HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. Edited by Victor P. Debattista and Cristina C. Popescu AIP Conferen

Physics

Optics

Black Holes, Globular Star Clusters, Adaptive Optics, Photometry, Mass, Galactic Nuclei, Circumnuclear Matter, And Bulges, Globular Clusters In External Galaxies, Adaptive And Segmented Optics, Photometric, Polarimetric, And Spectroscopic Instrumentation, Masses And Mass Distribution

Scientific paper

In this study, we present kinematics of the very centers of Omega Centauri and 47 Tucanae, obtained on the VLT using Fabry-Perot observations behind an adaptive optics system. The Fabry-Perot technique provides a unique tool to probe the central regions of crowded fields. Combined with HST photometry, these data are compared to dynamical models of the central regions of the clusters, setting constraints on the central black hole masses.

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