Fig. 7 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. 7.

Full‐resolution (VLBA plus HALCA) image of NGC 4261 at 4.9 GHz. The contours are −1.5%, 1.5%, 3%, 5%, and intervals of 5% up to 75%, plus and 85% and 95% of the peak (80 mJy beam⁻¹), and the restoring beam is ﹩2.82\times 1.14﹩ mas with the major axis along position angle −4﹩\fdg﹩6. The total flux density in the image is 388 mJy.

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