The Colour-Magnitude Relation and the Age of Galaxies in the Cluster AC118 at z=0.31

Simple item page
dc.creatorMerluzzi, P.
dc.creatorBusarello, G.
dc.creatorMassarotti, M.
dc.creatorLa Barbera, F.
dc.date2001-10-15
dc.date.accessioned2026-07-07T02:00:49Z
dc.date.available2026-07-07T02:00:49Z
dc.descriptionWe derive the Colour-Magnitude (CM) relation for the galaxy cluster AC118 at z=0.31 and use this relation to set constraints on the formation epoch and on the age spread of cluster galaxies in the framework of the passive evolution scenario. This work is based on observations at ESO NTT (OAC guaranteed time).
dc.description2 pages, 2 figures. To appear in ASP Conference Series: Proceeding of the Workshop "Tracing Cosmic Evolution with Galaxy Clusters"
dc.identifierhttps://arxiv.org/abs/astro-ph/0110328
dc.identifierhttp://arxiv.org/abs/astro-ph/0110328
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3538
dc.subjectAstrophysics
dc.titleThe Colour-Magnitude Relation and the Age of Galaxies in the Cluster AC118 at z=0.31
dc.typetext

Files

Collections

arXiv