Representation of kinematic components in the proper motions of stars using spherical functions

Details Representation of kinematic components in the proper motions of stars using spherical functions Representation of kinematic components in the proper motions of stars using spherical functions

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989velen.......73v&link_type=abstract

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia (ISSN 0024-0850), April 1989, p. 73-79. In Russian.

Statistics

Computation

Computational Astrophysics, Kinematics, Stellar Motions, Galactic Rotation, Least Squares Method, Legendre Functions

Scientific paper

Analytical expressions describing the effect of sun motion, galaxy rotation, and precession corrections in the proper motions of stars are expanded into a series in spherical functions. Explicit expressions are obtained for the first 68 coefficients, and their physical meaning is clarified. Relations describing the behavior of the series expansion coefficients are established.

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