A study of the core of the Shapley Concentration - I. The sample
Author(s) -
S. Bardelli,
E. Zucca,
G. Vettolani,
G. Zamorani,
R. Scaramella,
C. A. Collins,
H. T. MacGillivray
Publication year - 1994
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/267.3.665
Subject(s) - supercluster (genetic) , physics , astrophysics , galaxy cluster , redshift , galaxy , cluster (spacecraft) , brightest cluster galaxy , galaxy group , core (optical fiber) , sample (material) , abell 2744 , astronomy , biochemistry , chemistry , phylogenetics , thermodynamics , computer science , optics , gene , programming language
We report the first results of a spectroscopic survey of galaxies in the coreof the Shapley Concentration, the richest nearby supercluster of clusters ofgalaxies. We have measured 311 new galaxy redshifts in an area of $\sim 4.5$square degrees centered around the Abell cluster A3558. Considering also thedata already available in the literature, the total number of galaxy redshiftsin this area amounts to more than 500. On the basis of these data we estimatethe mean velocities and the velocity dispersions of the Abell clusters A3556,A3558 and the poor cluster SC 1329 -314. Finally, from an analysis of theprojected and three--dimensional distributions of galaxies in this region, weestimate the galaxy overdensity and find that the core of the ShapleyConcentration has an interesting, very complex dynamical state: the mainclusters appear to be interacting with each other, forming a single elongatedstructure containing many subcondensations.Comment: plain Tex, tables and figures upon request (contact BARDELLI@ALMA02.CINECA.IT) BAP 10-1993-030-DD
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom