Kinematic Analysis of Elliptical Galaxies Pairs

Details Kinematic Analysis of Elliptical Galaxies Pairs Kinematic Analysis of Elliptical Galaxies Pairs

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..26r.190f&link_type=abstract

XI IAU Regional Latin American Meeting of Astronomy (Eds. L. Infante & M. Rubio) Revista Mexicana de Astronomía y Astrofísica (S

Astronomy and Astrophysics

Astronomy

Scientific paper

We studied a sample of nearby elliptical galaxies pairs to correlate their kinematical properties in different environments and hosts systems. A sample of 150 pairs in the southern hemisphere were selected. The structural, kinematical and environmental properties of this population were classified. The statistical analysis allows us to conclude that elliptical galaxies pairs tend to be brighter and are more tightly bound than the mean system members when are located in high density systems.

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