Morphology and Dynamics of Galaxies

Details Morphology and Dynamics of Galaxies Morphology and Dynamics of Galaxies

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007padeu..19..203p&link_type=abstract

Publications of the Astronomy Department of the Eötvös University (PADEU), 2007, ISBN 963 463 557, Vol. 19. Edited by B. Érdi a

Astronomy and Astrophysics

Astronomy

Scientific paper

The determination of the galaxy interaction rate is obtained by measuring the incidence of strongly-disturbed galaxies or close pairs of galaxies. Photometrical data and HST/WFPC2 morphology of galaxies in dense environments of 3C 220.1 and 3C 34 radio galaxies are used in order to measure the rate of major galaxy merging/ interaction. In our study we determine the photometric redshifts of galaxies and we analyze the frequency of galaxies close pairs in the fields studied.

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