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Multi-Frequency VLBA+Effelsberg Observations of 1038+528 A/B

Published online by Cambridge University Press:  12 April 2016

M. J. Rioja  and
R. W. Porcas
M. J. Rioja
Affiliation:
Joint Institute for VLBI in Europe, Dwingeloo, Netherlands
R. W. Porcas
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany

Abstract

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We made a November 1995 observation of the close (33 arc sec) pair 1038+528 A,B using the VLBA+Effelsberg at 2.3 and 8.4 GHz, and the VLBA alone at 15 GHz. Our analysis of the precise astrometric separation between the core peak in A and a component ~ 1.8 mas from the core in B sheds new light on the observed changes with time and frequency.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 95 - 96
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Marcaide, J.M., & Shapiro, I.I. 1984. ApJ, 276, 56–59.Google Scholar
Rioja, M.J., et al. 1997. A&A, 325, 383–390.Google Scholar