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Simulation of Disk-Disk Encounters with Co-Moving Polar Grids

Published online by Cambridge University Press:  12 April 2016

Heikki Salo
Heikki Salo*
Affiliation:
Observatory, University of Helsinki, Finland

Abstract

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

Type
VII. Classical Theory of Pairs
Information
International Astronomical Union Colloquium , Volume 124: Paired and Interacting Galaxies , 1990 , pp. 595 - 599
Copyright
Copyright © NASA 1990

References

Miller, R.: 1976, J. Comp. Phys. 21, 400.Google Scholar
Noguchi, M.: 1987, M.N.R.a.S. 228, 635.Google Scholar
Noguchi, M.: 1988, Astron. Astrophys. 203, 259.Google Scholar
Salo, H.: 1987, Icarus 70, 37.Google Scholar
Salo, H.: 1990a, submitted to Icarus.Google Scholar
Salo, H.: 1990b, submitted to Astron. Astrophys.Google Scholar
Wisdom, J. and Tremaine, S.: 1988, A.J. 95, 925 Google Scholar