Surface Brightness of 38 Gal. Globular Clusters

DOI

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.

Cone search capability for table J/AJ/132/447/table1 (Clusters studied)

Identifier
DOI http://doi.org/10.26093/cds/vizier.51320447
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AJ/132/447
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/132/447
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/132/447
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AJ/132/447
Provenance
Creator Noyola E.; Gebhardt K.
Publisher CDS
Publication Year 2006
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy