Analysis of Two Strongly Interacting Galaxy Systems

Details Analysis of Two Strongly Interacting Galaxy Systems Analysis of Two Strongly Interacting Galaxy Systems

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..apr.c9014l&link_type=abstract

American Physical Society, April Meeting, 2003, April 5-8, 2003 Philadelphia, Pennsylvania, MEETING ID: APR03, abstract #C9.014

Physics

Scientific paper

We present numerical models of the Ring Galaxies, NGC 2793 and AM0644-741 (Linsay-Shapely Ring), based upon combined N-body/Smooth Particle Hydrodynamics simulations of collisions between a disk galaxy and an elliptical. The simulation results are compared to multiwavelength observations of these two systems, including HI and optical maps, to constrain the models and to investigate the history of impact-induced star formation, the disposition of cool gas, and the evolving velocity diastribution within the disturbed systems. We acknowledge support of DOE-LLNL contract B506657.

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