N-Body Simulations of Disk Galaxy Interactions

Details N-Body Simulations of Disk Galaxy Interactions N-Body Simulations of Disk Galaxy Interactions

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aps..ses.hd008m&link_type=abstract

American Physical Society, 71st Annual Meeting of the Southeastern Section, 11-13 November, 2004, Oak Ridge, TN. MEETING ID: S

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Scientific paper

We present results of N-body simulations for two interacting disk galaxies. The simulated galaxies are initially modeled with parameters fitting observations of the Milky Way Galaxy. We use a four-component model of a disk, dark matter halo, spheroid, and central concentration. In our present simulations, we neglect the gas component and associated star formation. Among our analysis, we address the question of member transference from one galaxy to another. We also examine the rate of member ejections from each disk system and final configurations after the disk interactions.

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