2004/05/27 by A. Mercurio, G. Busarello, P. Merluzzi +3
Medicine · Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Brightest cluster galaxy #Elliptical galaxy #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy group #Interacting galaxy #Lenticular galaxy #Medicine #Physics #Population #Redshift #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20040324
published as Astron.Astrophys. 424 (2004) 79 · 20 pages, 9 figures, A&A in press
arxiv created 2004/05/27 · openalex publication_date 2004/08/13 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We analyse the properties of galaxy populations in the rich Abell cluster ABCG 209 at redshift 0.21, on the basis of spectral classification of 102 member galaxies. We take advantage of available structural parameters to study separately the properties of bulge-dominated and disk-dominated galaxies. The star formation histories of the cluster galaxy populations are investigated by using line strengths and the 4000 Å break, through a comparison to stellar population synthesis models. The dynamical properties of different spectral classes are examined in order to infer the past merging history of ABCG 209. The cluster is characterized by the presence of two components: an old galaxy population, formed very early ( 3.5), and a younger ( 1.2) population of infalling galaxies. We find evidence of a merger with an infalling group of galaxies occurred 3.5–4.5 Gyr ago. The correlation between the position of the young H-strong galaxies and the X-ray flux shows that the hot intracluster medium triggered a starburst in this galaxy population ~3 Gyr ago.