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A&A 450, 9-14 (2006)
DOI: 10.1051/0004-6361:20041635
Substructures in Abell clusters of galaxies
P. Flin and J. KrywultPedagogical University, Institute of Physics, ul. Swietokrzyska 15, 25-406 Kielce, Poland
e-mail: sfflin@cyf-kr.edu.pl
(Received 10 July 2005 / Accepted 18 November 2005)
Abstract
Aims.
We present the results of substructure detection on a large sample of Abell
clusters.
Methods.
We apply the wavelet transform to positions of galaxies in 183 Abell clusters.
The significance of the substructuring detected was determined using Monte Carlo
simulations on sets of 1000 randomly generated distributions of galaxies for
each cluster and wavelet scale.
Results.
62 of the investigated clusters are strongly substructured; the frequency of
occurrence of substructure is 0.34. The investigated clusters were classified
as unimodal, bimodal or complex systems. The clusters were divided into
clusters having substructures in the field of the cluster S
or in the
core region S
. The Kolmogorov-Smirnov test show no significant differences
at the level
in the distribution of clusters having S
and
S
substructures with redshift. Using a
test we found no correlation
between the existence of subclustering and the morphological type of galaxy
clusters.
Key words: galaxies: clusters: general
SIMBAD Objects
© ESO 2006
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