UBV photometry in NGC 6528 Virtual Observatory Resource

Authors

1. van den Bergh S.
2. Younger F.

Published by

CDS

Abstract

On the basis of its color-magnitude diagram NGC 6528 is one of the two most metal-rich globular clusters that have so far been found in the Galaxy. Such a conclusion is consistent with Morgan's metallic line-strength classification of the integrated spectrum of this cluster. The reddening of NGC 6528 is estimated to be E(B-V)=0.52+/-0.07, from which R=6.1kpc and Z=-0.4kpc.

Keywords

1. globular-star-clusters
2. visible-astronomy
3. Wide-band photometry

Bibliographic source Bibcode

1979AJ.....84.1305V

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/84/1305

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AJ/84/1305

Document Object Identifer DOI

doi:10.26093/cds/vizier.50841305

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/84/1305
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/84/1305
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/84/1305

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).