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The Binggeli effect

Published online by Cambridge University Press:  12 October 2016

M. Biernacka ,
E. Panko ,
W. Godłowski ,
K. Bajan  and
P. Flin
M. Biernacka
Affiliation:
Institute of Physics, Jan Kochanowski University, Kielce, Poland email: bmonika@ujk.edu.pl
E. Panko
Affiliation:
Kalinenkov Observatory, Nikolaev National University, Nikolaev, Ukraine
W. Godłowski
Affiliation:
Institute of Physics, Opole University, Opole, Poland
K. Bajan
Affiliation:
Mt. Suhora Observatory, Cracow Pedagogical University, Krakow, Poland
P. Flin
Affiliation:
Institute of Physics, Jan Kochanowski University, Kielce, Poland email: bmonika@ujk.edu.pl
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Abstract

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We found the alignement of elongated clusters of BM type I and III (the excess of small values of the Δθ angles is observed), having range till about 60 h−1Mpc. The first one is probably connected with the origin of supergiant galaxy, while the second one with environmental effects in clusters, originated on the long filament or plane.

Keywords

galaxy clusteralignment
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S308: The Zeldovich Universe: Genesis and Growth of the Cosmic Web , June 2014 , pp. 479 - 481
Copyright
Copyright © International Astronomical Union 2016 

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