Clusters of galaxies in the mid-infrared

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dc.creatorBiviano, A.
dc.creatorMetcalfe, L.
dc.creatorCoia, D.
dc.creatorMcBreen, B.
dc.creatorAltieri, B.
dc.creatorPerez-Martinez, R.
dc.creatorSanchez-Fernandez, C.
dc.date2004-06-16
dc.date.accessioned2026-07-07T02:13:32Z
dc.date.available2026-07-07T02:13:32Z
dc.descriptionWe 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.
dc.descriptionTo 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0406365
dc.identifierhttp://arxiv.org/abs/astro-ph/0406365
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7847
dc.subjectAstrophysics
dc.titleClusters of galaxies in the mid-infrared
dc.typetext

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