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 Journal553968.
Provider: AAS Journals
Caption: Fig. 8.
Edited and selfâcalibrated 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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