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Determination of Absolute Proper Motions by Use of Automated Measurements of Tautenburg Plates
Published online by Cambridge University Press: 19 July 2016
Abstract
From measurements of Tautenburg Schmidt plates with the APM in Cambridge positional accuracies per plate of 0.″05 for stars and of 0.″10 for galaxies were achieved. With 0.″3/100a accuracy in a single stellar proper motion we obtained the absolute proper motion of the M3 globular cluster in good agreement between the two pairs of plates used.
- Type
- Part 4: Realization and comparison of reference frames
- Information
- Symposium - International Astronomical Union , Volume 141: Inertial Coordinate System on the Sky , 1990 , pp. 451 - 452
- Copyright
- Copyright © Kluwer 1990
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