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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. 12.

Brightness profile along the radio axis of NGC 4261 at 8.4 GHz, convolved with the same beam as in Fig. 11

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