Figure 2 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 2.

Free parameter variation along changing b _height. The thinner models are preferred by both of our millimeter wavelength images, based on the posterior values. However, thin disk models cannot explain the mid-infrared fluxes (Figure 3).

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