Fig. 3 from In the Shadow of the Accretion Disk: Higher Resolution Imaging of the Central Parsec in NGC 4261

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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. 3.

VLBA image of NGC 4261 at 1.6 GHz. The contours are 1%, 2%, and 5% followed by steps of 5% of the peak (64 mJy beam⁻¹). The restoring beam is ﹩12.73\times 4.62﹩ mas with major axis along position angle −23﹩\fdg﹩6.

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