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In the Shadow of the Accretion Disk: Higher Resolution Imaging of the Central Parsec in NGC 4261

  • Authors: Dayton L. Jones, Ann E. Wehrle, B. Glenn Piner, and David L. Meier

Jones et al. 2001 The Astrophysical Journal 553 968.

  • Provider: AAS Journals

Caption: Fig. 8.

Edited and self‐calibrated visibility amplitudes (in Jy) plus amplitudes from model clean components (smooth lines) as a function of projected baseline length at 4.9 GHz.

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