Absorption-line strengths in Coma galaxies

DOI

We present stellar population parameters of 12 elliptical and S0 galaxies in the Coma cluster around and including the cD galaxy NGC 4874, based on spectra obtained using the Low Resolution Imaging Spectrograph on the Keck II Telescope. Our data are among the most precise and accurate absorption-line strengths yet obtained for cluster galaxies, allowing us to examine in detail the zero-point and scatter in the stellar population properties of Coma cluster early-type galaxies (ETGs).

Cone search capability for table J/MNRAS/386/715/galaxies (The 187 galaxies with index strengths)

Identifier
DOI http://doi.org/10.26093/cds/vizier.73860715
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/386/715
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/386/715
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/386/715
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/386/715
Provenance
Creator Trager S.C.; Faber S.M.; Dressler A.
Publisher CDS
Publication Year 2009
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