Triaxiality and pressure anisotropy induced by tidal interactions between galaxies

Details Triaxiality and pressure anisotropy induced by tidal interactions between galaxies Triaxiality and pressure anisotropy induced by tidal interactions between galaxies

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sssmp..29.1073s&link_type=abstract

Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 29, Oct. 1986, p.

Statistics

Computation

Celestial Mechanics, Galactic Evolution, Gravitational Effects, Interacting Galaxies, Tides, Anisotropy, Fast Fourier Transformations, Point Sources, Rotating Spheres, Spheroids

Scientific paper

The response of a rotating Maclaurin spheroid to a close encounter with
a rapidly moving point mass is examined for the relation between the
shape, rotation and pressure anisotropy. The spheroid is simulated with
20,000 stars in a collision-free system and the self-consistent solution
obtained computationally by using fast Fourier transform methods.

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