UBV and proper motions of Palomar 13 Virtual Observatory Resource

Authors

1. Siegel M.H.
2. Majewski S.R.
3. Cudworth K.M.
4. Takamiya M.

Published by

CDS

Abstract

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

Keywords

1. Globular star clusters
2. CCD photometry
3. Optical astronomy
4. Wide-band photometry
5. Proper motions

Bibliographic source Bibcode

2001AJ....121..935S

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ivo://CDS.VizieR/J/AJ/121/935

Document Object Identifer DOI

doi:10.26093/cds/vizier.51210935

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