Fig. 3 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.

Caption: Fig. 3.

Core‐C1 (top), core‐C2 (middle), and core‐C3 (bottom) separations as a function of time, from 8.4 GHz model‐fitting analyses.