The kinematics of 512 stars in the system of FK5

Details The kinematics of 512 stars in the system of FK5 The kinematics of 512 stars in the system of FK5

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.177..213v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 177, no. 1-2, March 1991, p. 213, 214.

Astronomy and Astrophysics

Astrophysics

Astrometry, Celestial Mechanics, Stellar Motions, Stellar Parallax, Astronomical Catalogs, Data Reduction, Galactic Rotation, Least Squares Method, Precession

Scientific paper

The proper motions of 512 stars reduced to the system of FK5 were used for the determination of the velocity components X, Y, Z or the solar motion, Oort's constants A, B, and corrections Delta-n, Delta-k to Newcomb's precession values. It was found that the transition from FK4 to FK5 gives negligible and unsignificant changes to all the determined quantities.

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