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- W2020002005 abstract "The IAU (1976) luni-solar precession constant was derived by Fricke from intensive study of the catalog of 512 FK4-FK4/Sup distant stars. At present, when the data from the catalog HIPPARCOS is available, it is helpful to reconsider Fricke's analysis. This paper presents a redetermination of precession based on the following new factors: (a) the accurate parallaxes of stars have been taken into account; (b) galactic rotation and other kinematics have been eliminated from the proper motions of 512 stars; (c) the systems of the FK5 and improved GC catalog were used in combination with the HIPPARCOS catalog; (d) a new method (the MOTOR) of studying stellar kinematics was used. This method is based on the decomposition of proper motions on a set of orthogonal functions. The MOTOR, in contrast to the commonly used Least Squares Procedure, provides a test for whether or not the model is compatible with the data. Derived corrections to the IAU (1976) luni-solar precession constant are consistent with the results..." @default.
- W2020002005 created "2016-06-24" @default.
- W2020002005 creator A5075774731 @default.
- W2020002005 date "2002-01-01" @default.
- W2020002005 modified "2023-09-25" @default.
- W2020002005 title "Contribution of hipparcos to the determination of precession" @default.
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- W2020002005 doi "https://doi.org/10.1080/10556790215588" @default.
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