Physical completeness of classical models of the rotation of the Galaxy

Details Physical completeness of classical models of the rotation of the Galaxy Physical completeness of classical models of the rotation of the Galaxy

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...74v&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, July-Aug. 1990, p. 74-82, 96. In Russian.

Statistics

Computation

Astronomical Models, Galactic Rotation, Milky Way Galaxy, Computational Astrophysics, Precession, Stellar Motions

Scientific paper

The paper examines the problem of deriving Galactic-rotation parameters,
solar-motion parameters, and precession corrections on the basis of the
Oort-Lindblad and the Ogorodnikov-Milne models of the Galactic rotation.
It is shown that the proper motions of 512 FK4 stars do not confirm the
differential rotation of the Galaxy.

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