The Core Dynamics of the Dense Globular Cluster NGC 6752

Details The Core Dynamics of the Dense Globular Cluster NGC 6752 The Core Dynamics of the Dense Globular Cluster NGC 6752

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004hst..prop10121b&link_type=abstract

HST Proposal ID #10121

Physics

Hst Proposal Id #10121 Galaxies

Scientific paper

NGC 6752 is one of the best-studied dense globular clusters, and a wide variety of intriguing and anomalous results have been obtained. We propose ACS imaging of the core of this cluster. This will increase the accuracy of our previous internal proper motion measurements by almost an order of magnitude, providing an unprecedented probe of the central potential. The data will also greatly increase the radial extent of previous work on the binary frequency and luminosity function of this cluster. Together, the data will provide a new level of constraints on the dynamics of a dense globular cluster.

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