1998/12/11 by S. Phillipps, Phillipps, S., J. B. Jones +9
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9812229
8 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
arxiv created 1998/12/11 · openalex publication_date 1998/12/11 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Recent 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.