Figure 3 from Variable Outer Disk Shadowing around the Dipper Star RXJ1604.3

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Variable Outer Disk Shadowing around the Dipper Star RXJ1604.3–2130

Authors: P. Pinilla, M. Benisty, J. de Boer, C.F. Manara, J. Bouvier, C. Dominik, C. Ginski, R.A. Loomis, and A. Sicilia Aguilar

2018 The Astrophysical Journal 868 85.

Provider: AAS Journals

Caption: Figure 3.

Lorentzian MCMC best fit of the radial profile overlap with the uncertainty of the data profile for each epoch as shown in Figure 2. Notice that the radial range changes from Figure 2, to emphasize the ring shape and the fitting. In addition, we also overlay the power-law fit using nonlinear least squares analysis and considering the data points beyond the peak.

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