Simulation of disk-disk encounters with co-moving polar grids

Details Simulation of disk-disk encounters with co-moving polar grids Simulation of disk-disk encounters with co-moving polar grids

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nascp3098..595s&link_type=abstract

In NASA, Marshall Space Flight Center, Paired and Interacting Galaxies: International Astronomical Union Colloquium No. 124 p 59

Statistics

Computation

Cartesian Coordinates, Computational Grids, Computerized Simulation, Disk Galaxies, Gravitational Fields, Interacting Galaxies, Polar Coordinates, Stars, Encounters, Halos

Scientific paper

The two-grid simulation method combining advantages of both polar and Cartesian mesh-codes is described. In addition to the stellar component reacting solely to gravitational forces, the gas component is included with dissipatively colliding particles. This allows fairly realistic simulation of planar encounters where both systems contain star plus gas disks.

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