Surface Brightness of 38 Gal. Globular Clusters Virtual Observatory Resource

Authors

1. Noyola E.
2. Gebhardt K.

Published by

CDS

Abstract

The Hubble Space Telescope (HST) allows us to study the central surface brightness profiles of globular clusters at unprecedented detail. We have mined the HST archives to obtain 38 WFPC2 images of Galactic globular clusters with adequate exposure times and filters, which we use to measure their central structure.

Keywords

1. globular-star-clusters
2. surface-photometry

Bibliographic source Bibcode

2006AJ....132..447N

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https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/132/447

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AJ/132/447

Document Object Identifer DOI

doi:10.26093/cds/vizier.51320447

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http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/132/447
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/132/447
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/132/447

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https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/132/447/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/132/447/table1?