Disentangling Interacting Galaxy Pairs and Entangling Them Back

Details Disentangling Interacting Galaxy Pairs and Entangling Them Back Disentangling Interacting Galaxy Pairs and Entangling Them Back

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..390..186f&link_type=abstract

Pathways Through an Eclectic Universe ASP Conference Series, Vol. 390, proceedings of the conference held 23-27 April, 2007 at S

Mathematics

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Two-dimensional kinematics of disk galaxies give valuable information on the structure and evolution of these systems, complementing--sometimes contradicting--information derived from morphological studies. We present two cases of the use of two-dimensional kinematic information to study the interacting stage of galaxies. The first case portrays an apparently isolated local galaxy. The other points out the effects that higher redshifts--and thus the lack of spatial resolution--might have on the interpretation of this type of data.

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