Spectroscopic indexes of BCGs

DOI

This paper is part of a series devoted to the study of the stellar populations in brightest cluster galaxies (BCGs), aimed at setting constraints on the formation and evolution of these objects. We have obtained high signal-to-noise ratio, long-slit spectra of 49 BCGs in the nearby Universe. Here, we derive single stellar population (SSP)-equivalent ages, metallicities and alpha-abundance ratios in the centres of the galaxies using the Lick system of absorption line indices.

Cone search capability for table J/MNRAS/398/133/tabled (Index measurements for all the galaxies in the sample)

Identifier
DOI http://doi.org/10.26093/cds/vizier.73980133
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/398/133
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/398/133
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/398/133
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/398/133
Provenance
Creator Loubser S.I.; Sanchez-Blazquez P.; Sansom A.E.; Soechting I.K.
Publisher CDS
Publication Year 2010
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; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics