Galactic Kinematics Derived from Data in the RAVE5, UCAC4, PPMXL, and
  Gaia TGAS Catalogs
  The spatial velocities of the stars with high-precision positions, proper
motions and parallaxes from the Gaia TGAS catalog and line-of-sight velocities
from the RAVE5 catalog are considered. From the sample of 92395 stars with the
age estimates we have obtained the following kinematic parameters:
(U,V,W)=(9.42,20.34,7.21)+/-0.12,0.10,0.09) km/s, \Omega=26.29+/-0.39 km/s/kpc
and \Omega'=-3.89+/-0.08 km/s/kpc^2, where V0=210+/-6 km/s (for adopted
R0=8.0+/-0.2 kpc), and the Oort constants A=15.57+/-0.31 km/s/kpc and
B=-10.72+/-0.50 km/s/kpc. It is shown that the parameters \Omega and \Omega'
are stable to the star age. A comparative analysis of the Bottlinger model
parameters obtained separately from the RAVE5 catalog line-of-sight velocities
and the Gaia TGAS, UCAC4 and PPMXL catalogs proper motion has been made. It is
shown that these parameters are in good agreement with each other when derived
from the proper motions of both the terrestrial catalogs and catalog Gaia TGAS.
At the same time, it was established that the values of the Bottlinger model
parameters obtained from the line-of-sight velocities can differ from the
corresponding parameters obtained from the proper motions. The reduction of the
line-of-sight velocities from the RAVE5 catalog is proposed for eliminating
these differences.
