UBV and proper motions of Palomar 13

DOI

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.

Cone search capability for table J/AJ/121/935/table34 (Astrometry and photometry catalog)

Identifier
DOI http://doi.org/10.26093/cds/vizier.51210935
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AJ/121/935
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/121/935
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/121/935
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AJ/121/935
Provenance
Creator Siegel M.H.; Majewski S.R.; Cudworth K.M.; Takamiya M.
Publisher CDS
Publication Year 2005
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy