RX J105453.3+552102 cluster SDSS photometry

DOI

The most accepted scenario for the origin of fossil groups is that they are galaxy associations in which the merging rate was fast and efficient. These systems have assembled half of their mass at early epoch of the Universe, subsequently growing by minor mergers, and therefore could contain a fossil record of the galaxy structure formation. We have started an observational project in order to characterize a large sample of fossil groups. In this paper we present the analysis of the fossil system RX J105453.3+552102.

Cone search capability for table J/A+A/527/A143/table1 (Photometric and kinematic properties of the galaxies observed with DOLORES)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35270143
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/527/A143
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/527/A143
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/527/A143
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/527/A143
Provenance
Creator Aguerri J.A.L.; Girardi M.; Boschin W.; Barrena R.; Mendez-Abreu J.,Sanchez-Janssen R.; Borgani S.; Castro-Rodriguez N.; Corsini E.M.,Del Burgo C.; D'Onghia E.; Iglesias-Paramo J.; Napolitano N.; Vilchez J.M.
Publisher CDS
Publication Year 2011
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; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics