Volume 556, August 2013
|Number of page(s)||9|
|Published online||31 July 2013|
NoSOCS in SDSS
III. The interplay between galaxy evolution and the dynamical state of galaxy clusters
1 Laboratório de Astrofísica Teórica e Observacional, Departamento de Ciências Exatas e Tecnológicas, Universidade Estadual de Santa Cruz, 45650-000 Ilhéus-BA, Brazil
2 Observatório do Valongo, Universidade Federal do Rio de Janeiro, 20080-090 Rio de Janeiro-RJ, Brazil
3 Universidade Federal de Santa Maria, 97105-900 Santa Maria-RS, Brazil
Received: 28 November 2012
Accepted: 9 June 2013
Context. We investigate relations between the color and luminosity distributions of cluster galaxies and the evolutionary state of their host clusters.
Aims. Our aim is to explore some aspects of cluster galaxy evolution and the dynamical state of clusters as two sides of the same process.
Methods. We used 10 721 member galaxies of 183 clusters extracted from the Sloan Digital Sky Survey using a list of NoSOCS and CIRS targets. First, we classified the clusters into two categories, Gaussian and non-Gaussian, according to their velocity distribution measurements, which we used as an indicator of their dynamical state. We then used objective criteria to split up galaxies according to their luminosities, colors, and photometric mean stellar age. This information was then used to evaluate how galaxies evolve in their host clusters.
Results. Meaningful color gradients, i.e., the fraction of red galaxies as a function of radius from the center, are observed for both the Gaussian velocity distribution and the non-Gaussian velocity distribution cluster subsamples, which suggests that member galaxy colors change on a shorter timescale than the time needed for the cluster to reach dynamical equilibrium. We also found that larger portions of fainter red galaxies are found, on average, in smaller radii. The luminosity function in Gaussian clusters has a brighter characteristic absolute magnitude and a steeper faint-end slope than it does in the non-Gaussian velocity distribution clusters.
Conclusions. Our findings suggest that cluster galaxies experience intense color evolution before virialization, while the formation of faint galaxies through dynamical interactions probably takes place on a longer timescale, possibly longer than the virialization time.
Key words: galaxies: clusters: general / galaxies: evolution
© ESO, 2013
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