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High Precision Differential Astrometry in Large Angular Separation Pairs of Radiosources
Published online by Cambridge University Press: 19 July 2016
Abstract
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We show preliminary results of three of the four radiosource pairs with angular separations ranging from 0.01° to 6° where we have determined such a separation with a typical fractional precision of 10−8 using phase delays corrected for structural and ionospheric contributions. In the radiosource 4C39.25 we measure a motion with respect to an external radiosource which is compatible with previously reported internal superluminal motion.
- Type
- Astrometry
- Information
- Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 445 - 447
- Copyright
- Copyright © Kluwer 1994
References
Elósegui, P., et al. 1993, in Sub Arcsecond Radio Astronomy, ed. Davis, R. and Booth, R.S., Cambridge University Press,
(in press).
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