Environmental Effects on the Faint End of the Luminosity Function

Simple item page
dc.creatorPhillipps, S.
dc.creatorJones, J. B.
dc.creatorSmith, R. M.
dc.creatorCouch, W. J.
dc.creatorDriver, S. P.
dc.date1998-12-11
dc.date.accessioned2026-07-07T02:29:36Z
dc.date.available2026-07-07T02:29:36Z
dc.descriptionRecent studies have demonstrated that many galaxy clusters have luminosity functions (LFs) which are steep at the faint end. However, it is equally clear that not all clusters have identical LFs. In this paper we explore whether the variation in LF shape correlates with other cluster or environmental properties.
dc.description8 pages, LaTeX (uses ASP Conference Series paspconf.sty style file, included), with two embedded postscript figures, to appear in `The Low Surface Brightness Universe', Proceedings of I.A.U. Colloquium No. 171, Cardiff, eds. J. I. Davies, C. D. Impey & S. Phillipps, publ. Astronomical Society of the Pacific
dc.identifierhttps://arxiv.org/abs/astro-ph/9812229
dc.identifierhttp://arxiv.org/abs/astro-ph/9812229
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13536
dc.subjectAstrophysics
dc.titleEnvironmental Effects on the Faint End of the Luminosity Function
dc.typetext

Files

Collections

arXiv