Cosmological galaxy formation

Simple item page
dc.creatorPearce, F. R.
dc.creatorFrenk, C. S.
dc.creatorJenkins, A.
dc.creatorColberg, J. M.
dc.creatorThomas, P. A.
dc.creatorCouchman, H. M. P.
dc.creatorWhite, S. D. M.
dc.creatorEfstathiou, G.
dc.creatorPeacock, J. A.
dc.creatorNelson, A. H.
dc.date1999-06-02
dc.date.accessioned2026-07-07T02:31:47Z
dc.date.available2026-07-07T02:31:47Z
dc.descriptionWe discuss the first results from two successful simulations of galaxy formation within a cosmological volume. With over 2000 large objects forming in each we have sufficient numbers to reliably produce both galaxy correlation and luminosity functions. We find that the observed galaxy counts are well fitted by these models and that the galaxies display an almost un-evolving correlation function back to a redshift of 3 which closely resembles the featureless observed form and amplitude.
dc.description4 pages, Proceedings X Rencontres de Blois: The Birth of Galaxies
dc.identifierhttps://arxiv.org/abs/astro-ph/9906032
dc.identifierhttp://arxiv.org/abs/astro-ph/9906032
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14282
dc.subjectAstrophysics
dc.titleCosmological galaxy formation
dc.typetext

Files

Collections

arXiv