Figure 6 from Resolving the Circumstellar Disk of HL Tauri at Millimeter Wavelengths

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Resolving the Circumstellar Disk of HL Tauri at Millimeter Wavelengths

Authors: Woojin Kwon, Leslie W. Looney, and Lee G. Mundy

Kwon, Looney, & Mundy 2011 The Astrophysical Journal 741 3.

Provider: AAS Journals

Caption: Figure 6.

Posterior distributions of parameters in HL Tau. The solid lines of the plots indicate normal distributions of the posterior-weighted means and standard deviations of the parameter distributions. The posterior-weighted means and standard deviations are listed in Table 1 with the parameter search ranges.

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