• Benoist, Christophe
• Maurogordato, Sophie
• Schindler, Sabine
• Ferrari, Chiara
• Höller, Harald
• Pranger, Florian
• Böhm, Asmus

Abstract

Context. We present a spectrophotometric analysis of the galaxy population in the area of the merging cluster Abell 2384 at z = 0.094. <BR /> Aims: We investigate the impact of the complex cluster environment on galaxy properties, such as colour, morphology, and star formation rate. <BR /> Methods: We combined multi-object spectroscopy from the 2dF and EFOSC2 spectrographs with optical imaging of the inner 30 × 30 arcmin of A2384 taken with the ESO Wide Field Imager. We carried out a kinematical analysis using the EMMIX algorithm and biweight statistics. We address the possible presence of cluster substructures with the Dressler-Shectman test. Cluster galaxies are investigated with respect to [OII] and Hα equivalent width. Galaxies covered by our optical imaging observations are additionally analysed in terms of colour, star formation rate, and morphological descriptors, such as Gini coefficient and M<SUB>20</SUB> index. We study cluster galaxy properties as a function of clustercentric distance and investigate the distribution of various galaxy types in colour-magnitude and physical space. <BR /> Results: The Dressler-Shectman test reveals a substructure in the east of the 2dF field of view. We determine the mass ratio between the northern and southern subclusters to be ≲1.6:1. In accordance with other cluster studies, we find that a large number of the disk galaxies close to the cluster core show no detectable star formation (SF). Probably these are systems that are quenched by ram-pressure stripping. The sample of quenched disks populates the transition area between the blue cloud and the red sequence in colour-magnitude space. We also find a population of morphologically distorted galaxies in the central cluster region. <BR /> Conclusions: The substructure east of A2384 might be a group of galaxies falling onto the main cluster. We speculate that our sample of quenched spirals represents an intermediate phase in the ram-pressure-driven transformation of infalling field spirals into cluster S0s. This is justified by their position in colour-magnitude space. The occurrence of morphologically distorted galaxies in the cluster core complies with the hypothesis of Abell 2384 representing a post merger system. <P />The reduced spectra are only available in electronic form at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr">http://cdsarc.u-strasbg.fr</A> (ftp://130.79.128.5) or via <A href="http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/570/A40">http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/570/A40</A>...

Topics

• impedance spectroscopy
• cluster
• phase