1998/02/10 by R. Fusco-Femiano, R. Fusco‐Femiano, N. Menci · 17 citations
Mathematics · Physics and Astronomy · #Astrophysics #Binary number #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Intergalactic travel #Luminosity #Mathematics #Observable #Parameter space #Physics #RADIUS #Redshift #Space (punctuation) #Statistics #Velocity dispersion #astro-ph
paper · pdf · doi:10.1086/305536
published in The Astrophysical Journal 498(1), 95-105 (IOP Publishing) · 14 pages, Latex, 6 Figures and 2 Tables in Postscript. To appear in Astrophysical Journal Part1
arxiv created 1998/02/10 · openalex publication_date 1998/05/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/08
We compute the evolution of the space-dependent mass distribution of galaxies in clusters that arise from binary aggregations by solving a space-dependent Smoluchowski equation. From the solutions, we derive the distribution of intergalactic distances for different ranges of mass (and corresponding magnitudes). We compare the results with the observed distributions and find that the different degrees of luminosity segregation observed in clusters are well accounted for by our merging model. In addition, the presence of luminosity segregation is related to dynamical effects that also show up in different but connected observables, such as galaxy velocity profiles that decrease toward the center and X-ray-measured β-parameters smaller than 1. We predict that both luminosity segregation and the observables above (being a product of binary aggregations) are inversely correlated with the core radius and with the galaxy velocity dispersion; we also discuss how the whole set of predictions compares with up-to-date observations.