Accurate Internal Proper Motions in the Globular Cluster 47 Tucanae

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Hst Proposal Id #7993 Stellar Astrophysics

Scientific paper

We will measure internal proper motions of stars in 47 Tuc to an unprecedentedly high accuracy--error per star about 1/5 of the internal velocity dispersion in the cluster. In addition to images already secured by Meylan in 1995 and 1997 {GO-5912, 6467}, we will use archival images going back to 1991, which will greatly increase the overall accuracy. We demonstrate herein our ability to measure accurate proper motions from both WFPC-1 and WFPC2 material. The dispersion of proper motions, when compared with the known dispersion in radial velocities, will yield a far more accurate distance for the cluster than has been available until now.

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