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The Tautenburg Part Of The Programme Studying The Main Meridional Section Of The Galaxy

Published online by Cambridge University Press:  03 August 2017

E. Schilbach*
Affiliation:
Zentralinstitut für Astrophysik, R.-Luxemburg-Str. 17a, 1591 Potsdam, DDR

Abstract

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The programme for the determination of proper motions with reference to galaxies for 6000 stars on 17 fields near the main meridional section of the Galaxy is presented. For each field there are 2 or 3 first-epoch plates taken with the Tautenburg Schmidt-telescope before 1970. In preliminary investigations the mean error of an individual proper motion was found to be per century both for bright (8m–12m) and for faint (16m–18m) stars.

Type
Part II: Current Research
Copyright
Copyright © Kluwer 1988 

References

Kharchenko, N. V.: 1983, Astrometrija i Astrofizika (Kiev), 49, 61.Google Scholar
Maluto, V., Eelsalu, H., Jimsheleshvili, G.: 1981, Preprint A–2, Tartu.Google Scholar
Schilbach, E.: 1982, Astron. Nachr. 303, 6, 335.CrossRefGoogle Scholar
Scholz, R.-D. and Rybka, S. P.: 1987, Astron. Nachr., in press.Google Scholar