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A&A 403, 847-856 (2003)
DOI: 10.1051/0004-6361:20030441
Substructures and galaxy orientations in clusters II. Cluster Abell 14
F. W. Baier1, W. Godlowski2 and H. T. MacGillivray31 Institute for Communication and Structure Research, G.-Hauptmann-Str. 16, 14558 Bergholz-Rehbrücke, Germany
2 Jagellonian University, Astronomical Observatory, ul. Orla 171, 30-244 Krakow, Poland
3 Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, Scotland, UK
(Received 22 December 2000 / Accepted 27 February 2003)
Abstract
We present an investigation of the Abell 14 galaxy cluster, including a discussion
of subclustering, some aspects concerning its evolution, as well as
an analysis of galaxy orientations in the cluster
region. We confirm the previous results showing evidence for subclustering
in this cluster obtained from studies of galaxy distributions.
In this light, our aim has been to examine non-random
effects in the galaxy orientations in rich clusters, with
particular regard to the presence of subclustering. Our results
do provide evidence for non-random alignment of the galaxies in Abell 14
and confirm the presence of subclustering within this cluster. However,
the direction of the alignment is different from that (we) found for Abell 754
(Godlowski et al. 1998).
We continue our investigations by studying other clusters
in a similar manner. The results will be published in the next paper.
Key words: methods: statistical -- galaxies: clusters: general -- galaxies: clusters: individual: Abell 14
Offprint request: W. Godlowski, godlows@oa.uj.edu.pl
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© ESO 2003
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