Galaxies in the Perseus cluster field

DOI

We investigate the galaxies brighter than B~20 in the field of the Perseus cluster. The galaxies were selected on Schmidt CCD images in B and Halpha in combination with SDSS images. The survey field roughly covers the virial radius of the cluster. The galaxy sample is used for analysing cluster properties, such as radial profiles, indications of sub-structure, virial mass, and viral radius and is applied for a study of the cluster galaxy population with an emphasis on morphological types and peculiarities, star formation rates and active galactic nuclei.

Cone search capability for table J/A+A/640/A30/catalog (Galaxies in Perseus field)

Identifier
DOI http://doi.org/10.26093/cds/vizier.36400030
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/640/A30
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/640/A30
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/640/A30
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/640/A30
Provenance
Creator Meusinger H.; Rudolf C.; Stecklum B.; Hoeft M.; Mauersberger R.; Apai D.
Publisher CDS
Publication Year 2020
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; High Energy Astrophysics; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics