The structure and dynamics of the AC114 galaxy cluster revisited

TL;DR

This paper provides a detailed dynamical analysis of galaxy cluster AC114, including new velocity data, improved cluster parameters, and insights into its structure, galaxy populations, and mass, contributing to understanding cluster evolution.

Contribution

The study offers new velocity measurements, refined dynamical properties, and detailed structural analysis of AC114, enhancing previous knowledge of its mass, galaxy distribution, and internal dynamics.

Findings

Mean redshift z=0.31665 +/- 0.0008

Velocity dispersion σ=1893+73-82 km/s

Mass M_{200}= (4.3 ± 0.7) x 10^15 Msun/h

Abstract

We present a dynamical analysis of the galaxy cluster AC114 based on a catalogue of 524 velocities. Of these, 169 (32%) are newly obtained at ESO (Chile) with the VLT and the VIMOS spectrograph. Data on individual galaxies are presented and the accuracy of the measured velocities is discussed. Dynamical properties of the cluster are derived. We obtain an improved mean redshift value z= 0.31665 +/- 0.0008 and velocity dispersion \sigma= 1893+73-82 \kms. A large velocity dispersion within the core radius and the shape of the infall pattern suggests that this part of the cluster is in a radial phase of relaxation with a very elongated radial filament spanning 12000 \kms. A radial foreground structure is detected within the central 0.5/h Mpc radius, recognizable as a redshift group at the same central redshift value. We analyze the color distribution for this archetype Butcher-Oemler galaxy cluster and identify the separate red and blue galaxy sequences. The latter subset contains 44% of confirmed members of the cluster, reaching magnitudes as faint as R_{f}= 21.1 (1.0 magnitude fainter than previous studies). We derive a mass M_{200}= (4.3 \pm 0.7) x 10^15 Msun/h. In a subsequent paper we will utilize the spectral data presented here to explore the mass-metallicity relation for this intermediate redshift cluster.