Galaxy morphology in 5 medium redshift clusters Virtual Observatory Resource

Authors

1. Ascaso B.
2. Aguerri J.A.L.
3. Moles M.
4. Sanchez-Janssen R.
5. Bettoni D.

Published by

CDS

Abstract

Following the study presented in our previous paper, based on the Nordic Optical Telescope (NOT) sample, which consists of five clusters of galaxies within the redshift range 0.18<=z<=0.25 imaged in the central 0.5-2Mpc in very good seeing conditions, we have studied the quantitative morphology of their bright galaxy population. We analyzed the surface brightness profiles of the galaxy population in those clusters, after performing simulations in order to check the reliability of the fits. We also derived a quantitative morphological classification.

Keywords

1. Galaxy clusters
2. Galaxies
3. Photometry
4. Galaxy classification systems

Bibliographic source Bibcode

2009A&A...506.1071A

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/506/1071

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/506/1071

Document Object Identifer DOI

doi:10.26093/cds/vizier.35061071

Access

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http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/506/1071

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