Surfaces of zero relative velocity in the gravitational field of a pair of interacting galaxies

Details Surfaces of zero relative velocity in the gravitational field of a pair of interacting galaxies Surfaces of zero relative velocity in the gravitational field of a pair of interacting galaxies

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..67..503s&link_type=abstract

Astrophysics and Space Science, vol. 67, no. 2, Feb. 1980, p. 503-510.

Astronomy and Astrophysics

Astrophysics

4

Astronomical Models, Disk Galaxies, Galactic Clusters, Gravitational Effects, Interacting Galaxies, Many Body Problem, Cartesian Coordinates, Gravitational Fields

Scientific paper

The theory for obtaining zero relative velocity surfaces for an infinitesimal particle moving in the gravitational field of two finite masses has been extended to a system consisting of an infinitesimal particle moving in the gravitational field of two extended configurations of finite masses. Zero relative velocity surfaces in the orbital plane have been computed for close pairs of spherical and disk galaxies.

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