Colors, Ages, and Metallicities of Galaxies in Six Nearby Galaxy Clusters

Astronomy and Astrophysics – Astronomy

Scientific paper

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Galaxy Clusters : Individual (A1436, A1773, A1809, A2048, A2142, And A2152), Galaxy : Photometry, Galaxy : Color, Age, And Metallictiy, Galaxy : Formation And Evolution

Scientific paper

We present an optical-infrared photometric study of galaxies in six nearby clusters of galaxies at z=0.041˜0.098 (A1436, A1773, A1809, A2048, A2142, and A2152). Using BVI photometry obtained at the Bohyunsan Optical Astronomical Observatory and JHK_{S} photometry extracted from the 2-Micron All-Sky Survey catalog, we investigate the colors of galaxies in the clusters. Using the (B-V) versus (I-K_{S}) color-color diagrams in comparison with the simple stellar population model, we estimate the ages and metallicities of bright early-type member galaxies. Early-type galaxies in each cluster show the color-magnitude relation. Ages and metallicities of early-type members show little dependence on their velocity dispersions. Mean ages of early-types in the clusters range from 3 Gyr to 20 Gyr, showing a large dispersion, and mean metallicities range from Z=0.03 to 0.05 above the solar value, showing a negligible dispersion.

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