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We transformed radial velocities compiled from more than 1400 publishedsources, including the Geneva--Copenhagen survey of the solar neighborhood(CORAVEL-CfA), into a uniform system based on the radial velocities of 854standard stars in our list. This enabled us to calculate the average weightedradial velocities for more than 25~000 HIPPARCOS stars located in the localGalactic spiral arm (Orion arm) with a median error of +-1 km/s. We use theseradial velocities together with the stars' coordinates, parallaxes, and propermotions to determine their Galactic coordinates and space velocities. Thesequantities, along with other parameters of the stars, are available from thecontinuously updated Orion Spiral Arm CAtalogue (OSACA) and the associateddatabase. We perform a kinematic analysis of the stars by applying anOgorodnikov-Milne model to the OSACA data. The kinematics of the nearest singleand multiple main-sequence stars differ substantially. We used distant(r\approx 0.2 kpc) stars of mixed spectral composition to estimate the angularvelocity of the Galactic rotation -25.7+-1.2 km/s/kpc, and the vertexdeviation,l=13+-2 degrees, and detect a negative K effect. This negative Keffect is most conspicuous in the motion of A0-A5 giants, and is equal toK=-13.1+-2.0 km/s/kpc.Comment: 16 pages, 8 figure

The OSACA database and a kinematic analysis of stars in the solar neighborhood