Properties of Galactic Globular Clusters

We have assembled 560 recent measurements from the literature of distances of Galactic globular clusters and found revised distance estimates for 154 of the 157 clusters in the McMaster catalogue [Harris, 2010 edition, Cat. VII/202]. We find a trough in the X-distribution at the Galactic centre, and symmetries corresponding to the structure of the bar. These features indicate a distance, R_0_=7.4+/-0.2(stat)+/-0.2(sys)kpc, only a little higher than Bica et al.'s (2006, Cat. J/A+A/450/105) estimate.

Cone search capability for table VII/271/catalog (Properties of globular clusters)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/VII/271
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/VII/271
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=VII/271
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/VII/271
Provenance
Creator Francis C.; Anderson E.
Publisher CDS
Publication Year 2014
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; Exoplanet Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy