Newly identified star clusters in M 31 Virtual Observatory Resource

Authors

1. Krienke K.O.
2. Hodge P.W.

Published by

CDS

Abstract

Using the HST archives, we have searched portions of the southern half and northwest quarter of the Andromeda Galaxy (M 31, NGC 224) for previously unrecognized star clusters. The result is a table of the characteristics of 71 newly identified star clusters. Most are moderately faint, low-mass clusters. Absolute magnitudes range from M(V)=-6.3 to -2.5.

Keywords

1. galaxies
2. stellar-associations
3. hst-photometry

Bibliographic source Bibcode

2013PASP..125..636K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/125/636

IVOA Identifier IVOID

ivo://CDS.VizieR/J/PASP/125/636

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASP/125/636
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASP/125/636
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASP/125/636

IVOA Table Access TAP

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

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASP/125/636/table2?
https://vizier.iucaa.in/viz-bin/conesearch/J/PASP/125/636/table2?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASP/125/636/table2?