The Multiformity of the Evidence of Galaxy Interactions

Details The Multiformity of the Evidence of Galaxy Interactions The Multiformity of the Evidence of Galaxy Interactions

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..396..281m&link_type=abstract

Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the results of the spectral study of the some candidates to the polar-ring galaxies. New information about structure and kinematics of gaseous and stellar components was obtained using modern observing techniques such as integral field (3D) spectroscopy and high resolution long-slit spectroscopy. Detailed analysis of the data allowed us to conclude that investigated objects have complicated multi-component structure among which we can distinguish galaxies with classical polar rings, with circumnuclear polar disks, galaxies with warped gaseous disks and rings and even with stellar polar rings.

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