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The large-scale distribution of galaxies in the Shapley Concentration

1998/11/02 by S. Bardelli, E. Zucca, Bardelli, S. +3
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9811015

4 LATEX pages with 3 encapsulated figures; to appear in the proceedings of 'Observational Cosmology: The Development of Galaxy systems', Sesto 1998

arxiv created 1998/11/02 · openalex publication_date 1998/11/02 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We present the results of a galaxy redshift survey in the central region of the Shapley Concentration. Our total sample contains ~2000 radial velocities of galaxies both in the clusters and in the intercluster field. We reconstruct the density profile of this supercluster, calculate its overdensity and total mass. Moreover we detect a massive structure behind the Shapley Concentration, at ~30000 km/s.

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