Tracing cosmic evolution with the Coma cluster

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dc.creatorPoggianti, Bianca M.
dc.creatorBridges, Terry J.
dc.creatorMobasher, Bahram
dc.creatorCarter, Dave
dc.date2001-10-08
dc.date.accessioned2026-07-07T02:00:42Z
dc.date.available2026-07-07T02:00:42Z
dc.descriptionWe summarize here the first results of a new spectroscopic survey of galaxies in the Coma cluster with -20.5 < M_B < -14. Differences between the last epoch of star formation (SF) activity in S0 and elliptical galaxies are discussed. Furthermore, we show that about half of all galaxies without present-day SF display signs of activity at z < 1-2. Systematic trends of most recent SF epoch with galaxy luminosity are presented.
dc.description4 pages, to appear in the proceedings of the meeting "Tracing cosmic evolution with galaxy clusters" (Sesto Pusteria 3-6 July 2001), ASP Conference Series in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0110170
dc.identifierhttp://arxiv.org/abs/astro-ph/0110170
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3493
dc.subjectAstrophysics
dc.titleTracing cosmic evolution with the Coma cluster
dc.typetext

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