Fig. 4 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. 4.

Comparison of 8.4 GHz models from 1991 November 24 and 1992 March 26. The horizontal axes are coordinate axes in milliarcseconds, and the vertical axis is the flux density in Jy beam⁻¹ (scale not shown, but identical to the images in Fig. 2).

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