Luminosity Function of Early-Type Galaxies in Clusters Cores

dc.creatorMolinari, Emilio
dc.creatorSmareglia, Riccardo
dc.date1995-12-18
dc.date.accessioned2026-07-07T02:20:38Z
dc.date.available2026-07-07T02:20:38Z
dc.descriptionWe show the possibility to exploit the non-linear behaviour of artificial neural network (ANN) for the identification of the early-type component of the population of the core of clusters of galaxies. We result in a measurement of the luminosity function of the E/S0 galaxies which disfavours the hypothesis of a universal LF and calls for dynamical influences.
dc.description4 pages, uuencoded gzipped ps-file, 326 kByte Proc. ``Mapping, Measuring and Modelling the Universe'', Valencia 1995, eds.: P. Coles, V. Martinez, M. Pons, to be published by ASP
dc.identifierhttps://arxiv.org/abs/astro-ph/9512114
dc.identifierhttp://arxiv.org/abs/astro-ph/9512114
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10274
dc.subjectAstrophysics
dc.titleLuminosity Function of Early-Type Galaxies in Clusters Cores
dc.typetext

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