/ftp/cats/A+A/430/19



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J/A+A/430/19         VRI photometry of Abell 3921 galaxies     (Ferrari+, 2005)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	tablea.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/430/19
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Beginning of ReadMe : J/A+A/430/19 VRI photometry of Abell 3921 galaxies (Ferrari+, 2005) ================================================================================ Dynamical state and star formation properties of the merging galaxy cluster Abell 3921. Ferrari C., Benoist C., Maurogordato S., Cappi A., Slezak E. <Astron. Astrophys. 430, 19 (2005)> =2005A&A...430...19F ================================================================================ ADC_Keywords: Clusters, galaxy ; Redshifts ; Photometry, VRI ; Equivalent widths Keywords: galaxies: clusters: general - galaxies: clusters: individual: Abell 3921 - galaxies: distances and redshifts - cosmology: observations Abstract: We present the analysis and results of a new VRI photometric and spectroscopic survey of the central  1.8x1.2Mpc^2^ region of the galaxy cluster A3921 (z=0.094). We detect the presence of two dominant clumps of galaxies with a mass ratio of  5: a main cluster centred on the Brightest Cluster Galaxy (BCG) (A3921-A), and an NW sub-cluster (A3921-B) hosting the second brightest cluster galaxy. The distorted morphology of the two sub-clusters suggests that they are interacting, while the velocity distribution of 104 confirmed cluster members does not reveal strong signatures of merging. Description: The optical observations of Abell 3921 were carried out using the Wide Field Imager (WFI) mounted at the Cassegrain focus of the MPG/ESO 2.2m telescope at La Silla observatory. The data, including photometric calibration images, were obtained between August 20th and 23rd, 2001. Positions, V, R, I-band magnitudes (AB magnitude system), radial velocity measurements, and equivalent widths of [OII]3727AA and Hdelta lines of 239 objects in the central region of the galaxy cluster Abell 3921 are presented.