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Table · dataset · 2005

UBV and proper motions of Palomar 13

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We present a proper-motion, CCD photometric study of stars in the distant halo globular cluster Palomar 13.

Description

The absolute proper motion of Pal 13 with respect to the background galaxies, derived from moderate-scale photographic plates separated by a 40 year baseline, is (pmRAcosDE, pmDE)=(2.30, 0.27)+/-(0.26, 0.25)mas/yr.

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