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For refcode 1989MNRAS.237..341A:
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NED Abstract

Copyright by Royal Astronomical Society. 1989MNRAS.237..341A VLBI observations of the nuclei of a mixed sample of bright galaxies and quasars at 327 MHz S. Ananthakrishnan and V.K. Kulkarni Radio Astronomy Centre, Tata Institute of Fundamental Research, PO Box 8, Udhagamandalam 643001, India J.E.B. Ponsonby and R.E. Spencer University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL D.A. Graham and R.W. Porcas Max-Planck-Institut fur Radioastronomie, Auf dem Hugel 69, D-5300 Bonn, FRG A. Van Ardenne and R.T. Schilizzi Netherlands Foundation for Radio Astronomy, Postbus 2, 7990 AA Dwingeloo, The Netherlands S. Gorgolewski and A. Kus Torun Radio Astronomy Observatory, Torun, Poland L.I. Matveyenko and A.H. Papacenko Space Research Institute, Moscow, USSR Accepted 1988 September 12. Received 1988 August 9 Summary. We present the first VLBI observations using the Ooty telescope. An array consisting of telescopes at Ooty (India), Crimea (USSR), Torun (Poland), Westerbork (Netherlands) and Jodrell Bank (United Kingdom) was operated in 1983 December at a frequency of 327 MHz. Nearby galaxies, compact quasars and SS433 were observed in this pilot experiment. Most of the galaxies were found to be well resolved. The structure of SS433 (visible only on the shortest baseline) is consistent with that obtained in previous high-frequency VLBI work. The visibilities of the compact quasars indicate that large-scale scattering may be taking place in the interplanetary medium.
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