Spectroscopic indexes of BCGs (Loubser+, 2009)

Details Spectroscopic indexes of BCGs (Loubser+, 2009) Spectroscopic indexes of BCGs (Loubser+, 2009)

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..73980133l&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/398/133. Originally published in: 2009MNRAS.398..133L

Physics

Clusters: Galaxy, Spectroscopy

Scientific paper

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.
(2 data files).

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