Title:IFU study of the morphologically distorted galaxy Kaz364

Abstract:
We present preliminary results on the study of the morphologically distorted 
galaxy Kaz364, a probable member of a substructure of the galaxy cluster A85. 
The aim of this study is to disentangle the origin and importance of the 
environmental effects that are acting to produce this distortion, whether they 
are dominantly hydrodynamical or gravitational. We used IFU data obtained with 
the Eucalyptus spectrograph, on a 30''x15'' field covering the central region 
of the galaxy, supplemented by photometric data in various bands. We found a 
complex central kinematical pattern, probably dominated by the biconical 
emission from the broad line region of the AGN hosted on Kaz364. The pseudo-SED 
of the galaxy confirms the presence of dust, expected from the Sy2 nature of 
the AGN. The most striking feature seems to be the misalignment between the 
plane of the galaxy''s disk and the dust torus. We also present comparative 
results of the external effects from ram-pressure stripping, tidal interaction 
with the nearest neighbor and tidal interaction with the cluster''s potential 
well.