Fig. 1 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. 1.

VLBA image of NGC 4261 at 8.4 GHz. The contours increase in steps of ﹩\sqrt{2}﹩ starting at ±0.75% of the peak (99 mJy beam⁻¹). The restoring beam is ﹩1.86\times 0.79﹩ mas with major axis along position angle −1﹩\fdg﹩3.

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