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Five Years of Stellar Position Measurements with the MKIII Optical Interferometer
Published online by Cambridge University Press: 19 July 2016
Abstract
Using the north-south and east-south astrometric baselines of the MKIII optical interferometer on Mt. Wilson (each about 12 meters in length), we measured the positions of eleven EK5 stars with an accuracy of about 10 milliarcseconds (mas) in declination and 20 mas in right ascension.
- Type
- Astrometry
- Information
- Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 448 - 450
- Copyright
- Copyright © Kluwer 1994
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