Evolution of the Red Sequence in simulated galaxy groups

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dc.creatorRomeo, A. D.
dc.creatorNapolitano, N. R.
dc.creatorCovone, G.
dc.creatorSommer-Larsen, J.
dc.date2006-12-15
dc.date.accessioned2026-07-07T07:35:11Z
dc.date.available2026-07-07T07:35:11Z
dc.descriptionN--body + hydrodynamical simulations of formation and evolution of galaxy groups in a LambdaCDM cosmology have been performed. The properties of the galaxy populations in 12 groups are here discussed, with focus on the colour-magnitude relation in both normal and fossil groups.
dc.descriptionProceedings of the Conference "DEEP06 - At the edge of the Universe", Sintra, 9-13 October 2006; 5 pages, 3 colour figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0612423
dc.identifierhttp://arxiv.org/abs/astro-ph/0612423
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120014
dc.subjectAstrophysics
dc.titleEvolution of the Red Sequence in simulated galaxy groups
dc.typetext

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