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The kinematics of 512 stars in the system of FK5
Authors:V V Vityazev
Institution:(1) Petrodvorets Bibliotechnaya P1.2 Astronomical Observatory, Leningrad State University, 198904 Leningrad, USSR
Abstract:The proper motions of 512 stars reduced to the system of FK5 were used for the determination of the velocity components X,Y,Z of the solar motion, Dort's constants A,B, and corrections Deltan, Deltak 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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