2004/06/16 by A. Biviano, L. Metcalfe, Biviano, A. +11
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0406365
To appear in the Mem.S.A.It. Supplements, proceedings of the 48th meeting of the Italian Astronomical Society, eds.: A. Wolter, G. Israel, F. Bacciotti
arxiv created 2004/06/16 · arxiv updated 2009/12/01
We describe the results of observations of galaxy clusters conducted with ISOCAM on-board the Infrared Space Observatory. Our research is aimed at understanding the processes driving galaxy evolution in dense environments, free from the bias of dust extinction. The results reveal quite a complex picture: the star-formation activity of cluster galaxies does not show a simple evolution with redshift, but also depends on the dynamical status and evolutionary history of the clusters.