Statistics – Computation
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...309..472q&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 309, Oct. 15, 1986, p. 472-495.
Statistics
Computation
221
Celestial Mechanics, Galactic Structure, Many Body Problem, Orbital Mechanics, Spiral Galaxies, Angular Momentum, Circular Orbits, Computational Astrophysics, Disks, Radii, Temporal Distribution
Scientific paper
The interaction of a spiral galaxy with its system of satellites leads to the orbital decay of the satellites on time scales comparable to their orbital periods. Over a Hubble time, the disk of a spiral and the distribution of satellites can be significantly altered by the action of dynamical friction which leads to the exchange of mass and energy between the satellites and the disk. The authors have used a restricted N-body method to uncover the essential dynamics of friction in disk-satellite systems and to investigate the orbital decay rates as a function of the satellite's mass and orbital parameters.
Goodman Jeremy
Quinn Peter J.
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