/ftp/cats/aliases/O/OSACA



==========================================================================
J/AZh/83/821 Compiled stellar radial velocities catalog (OSACA) (Bobylev+, 2006)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	osaca.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/AZh/83/821
==========================================================================

drwxr-xr-x 8 cats archive 156 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 270 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 469 Dec 19 2022 .message -r--r--r-- 1 cats archive 5118 May 6 2020 ReadMe -rw-r--r-- 1 cats archive 1997 Nov 7 2007 +footg5.gif -rw-r--r-- 1 cats archive 35346 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 3129539 Aug 14 2007 osaca.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AZh/83/821 Orion Spiral Arm CAtalogue (OSACA) (Bobylev+, 2006) ================================================================================ The OSACA Database and a Kinematic Analysis of Stars in the Solar Neighborhood. Bobylev V.V., Goncharov G.A., Bajkova A.T. <Astron. Zh. 83, 821 (2006)> =2006AZh....83..821B =2006Arep..50...733B ================================================================================ ADC_Keywords: Radial velocities; Proper motions Abstract: We transformed radial velocities compiled from more than 1400 published sources, including the Geneva-Copenhagen survey of the solar neighborhood (2004, Nordstrom et al., Cat. V/117), into a uniform system based on the radial velocities of 854 standard stars in our list (Gontcharov, 2006, Cat. III/252 ). This enabled us to calculate the average weighted radial velocities for more than 25000 HIPPARCOS stars located in the local Galactic spiral arm (Orion arm) with a median error of 1km/s. We use these radial velocities together with the stars coordinates, parallaxes, and proper motions to determine their Galactic coordinates and space velocities. These quantities, along with other parameters of the stars, are available from the continuously updated Orion Spiral Arm CAtalogue (OSACA) and the associated database. We perform a kinematic analysis of the stars by applying an Ogorodnikov-Milne model to the OSACA data. The kinematics of the nearest single and multiple main-sequence stars differ substantially.