Figure 2 from Detecting Flaring Structures in Sagittarius A* with High-Frequency VLBI

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Detecting Flaring Structures in Sagittarius A* with High-Frequency VLBI

Authors: Sheperd S. Doeleman, Vincent L. Fish, Avery E. Broderick, Abraham Loeb, and Alan E. E. Rogers

DOELEMAN et al. 2009 The Astrophysical Journal 695 59.

Provider: AAS Journals

Caption: Figure 2.

Images of Model B. Columns show orbital phases 0, 0.2, 0.4, 0.6, and 0.8 from left to right. From top to bottom, rows show the input model at 230 GHz, the same model after convolution with expected interstellar scattering at 230 GHz, the model at 345 GHz, and the same model after scattering at 345 GHz.

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