Fig. 1 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. 1.

Contour levels for (a), (b), (c), (d), (e), (g), (i), (j), and (n)–(u) are −1, 1, 2, 4, 8, 16, 32, and 64 percent of the peak flux density in the map as given in Table 1. The contour levels for (f), (h), and (k)–(m) are −0.5, 0.5, 1, 2, 4, 8, 16, 32, and 64 percent of the peak flux densities as given in Table 1.

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