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Panchromatic Observations and Modeling of the HV Tau C Edge-on Disk

  • Authors: G. Duchêne, C. McCabe, C. Pinte, K. R. Stapelfeldt, F. Ménard, G. Duvert, A. M. Ghez, H. L. Maness, H. Bouy, D. Barrado y Navascués, M. Morales-Calderón, S. Wolf, D. L. Padgett, T. Y. Brooke, and A. Noriega-Crespo

DUCHÊNE et al. 2010 The Astrophysical Journal 712 112.

  • Provider: AAS Journals

Caption: Figure 11.

Bayesian inference probability distributions for the free parameters in our model, based on fitting the three scattered light images at once (dashed blue histograms), the SED (dot-dashed red), the spatially resolved 1.3 mm correlated fluxes (dotted green), and all observations at once (solid black). The probability distribution for the inclination based on the 1.3 mm is almost flat and very close to 0. For reference, the filled diamonds indicate the value of the parameters for the model with the absolute lowest χ 2 tot in our grid. Note the different vertical scale in the two rows of plots.

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