Dark Matter Haloes in Isolated Interacting Galaxy Pairs

Details Dark Matter Haloes in Isolated Interacting Galaxy Pairs Dark Matter Haloes in Isolated Interacting Galaxy Pairs

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17...44f&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Astronomy and Astrophysics

Astronomy

Galaxies: Kinematics, Galaxies: Interactions, Galaxies: Dark Matter, Galaxies: Spiral

Scientific paper

Most of the studies attempting to characterise the mass-to-luminosity ratio (M/L) and the structure of dark matter haloes in isolated interacting galaxy pairs have used a statistical approach of the problem. It is important though to restrain these parameters through the detailed observations and analysis of the kinematics and dynamics of specific interacting galaxy pairs. We present results on the preliminary study of the M-51 type interacting galaxy pair Kar302 (NGC 3893/96).

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