Fig. 2 from The Subparsec‐Scale Structure and Evolution of Centaurus A: The Nearest Active Radio Galaxy

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The Subparsec‐Scale Structure and Evolution of Centaurus A: The Nearest Active Radio Galaxy

Authors: S. J. Tingay, D. L. Jauncey, J. E. Reynolds, A. K. Tzioumis, E. A. King, R. A. Preston, D. L. Jones, D. W. Murphy, D. L. Meier, T. D. van Ommen, P. M. McCulloch, S. P. Ellingsen, M. E. Costa, P. G. Edwards, J. E. J. Lovell, G. D. Nicolson, J. F. H. Quick, A. J. Kemball, V. Migenes, P. Harbison, P. A. Jones, G. L. White, R. G. Gough, R. H. Ferris, M. W. Sinclair, and R. W. Clay

Tingay et al. 1998 The Astronomical Journal 115 960.

Provider: AAS Journals

Caption: Fig. 2.

Montage of 8.4 GHz VLBI images. Left: Series of clean component models from the 8.4 GHz SHEVE images. An average restoring beam of 9 mas × 3 mas in position angle −83° has been used for the SHEVE models. Right: Series of clean component models from the 8.4 GHz VLBA images. An average restoring beam of 4 mas × 13 mas in position angle 2° has been used for the VLBA models. All models and beams have been rotated by 39°. Note that the two panels displayed have significantly different scales, because of the timescales over which the observations were made.

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