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Stellar Kinematics in the Galactic North Pole Region on the Basis of Tautenburg Schmidt Telescope Plates

Published online by Cambridge University Press:  26 July 2016

N.V. Kharchenko ,
E. Schilbach  and
R.-D. Scholz
N.V. Kharchenko
Affiliation:
Main Astronomical Observatory of the Ukrainian Academy of Sciences, Kiev
E. Schilbach
Affiliation:
WIP - Projekt Astrometrie bei der Universität Potsdam, Germany
R.-D. Scholz
Affiliation:
WIP - Projekt Astrometrie bei der Universität Potsdam, Germany

Abstract

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The spatial velocity components and their dispersions in the Galactocentric and rotation directions, eccentricities of Galactic orbits, parameters of spatial distribution and the change of all these characteristics with distance from the Galactic plane are detennined. These data have been obtained on the basis of absolute proper motions and stellar B, V magnitudes in two sky regions near the North Galactic Pole (NGP) by means of a plate set of the Tautenburg Schmidt telescope.

Type
Part Nine: Galactic Structure
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 444 - 446
Copyright
Copyright © Kluwer 1994 

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