Stellar population trends in S0 galaxies (Chamberlain+, 2011)

Details Stellar population trends in S0 galaxies (Chamberlain+, 2011) Stellar population trends in S0 galaxies (Chamberlain+, 2011)

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74120423c&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/412/423. Originally published in: 2011MNRAS.412..423C

Physics

Galaxies: Photometry, Morphology, Abundances

Scientific paper

We present stellar population age and metallicity trends for a sample of 59 S0 galaxies based on optical Sloan Digital Sky Survey (SDSS) and near-infrared (NIR) J and H photometry. When combined with optical g and r passband imaging data from the SDSS archive and stellar population models, we obtain radial age and metallicity trends out to at least five effective radii for most of the galaxies in our sample. The sample covers a range in stellar mass and light concentration.
(6 data files).

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