1997/10/24 by H. Andernach, E. Tago, Andernach, H. +2
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9710265
4 pages; LaTeX; to appear in Proc. of "Large Scale Structure: Tracks and Traces", World Scientific Publ., Singapore, eds. V.Müller, S.Gottlöber, J.P.Mücket, & J.Wambsganss, held at Potsdam, Germany, Sept. 15-19, 1997
arxiv created 1997/10/24 · openalex publication_date 1997/10/24 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
We present an update of our compilation of measured redshifts of galaxy clusters in the all-sky Abell catalog. In the last 7 years the number of ACO clusters with measured z has doubled to now ~2100, but still ~56% of these are based on only 1 or 2 measured member galaxies. Our October 1997 version gives 2247 redshifts (including components or line-of-sight superpositions) for 2114 distinct A- and S-clusters. Velocity dispersions are listed for 536 different ACO clusters (613 subclusters) and the median is 695 km/s. We mention some applications of our compilation for determining the large-scale structure of the nearby Universe.