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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 3.

HL Tau SED overlaid with models of various b height values. The solid line is the case of b height = 1.5 and the dashed lines are cases of b height = 0.1, 0.2, 0.5, 1.0, and 2.0 from the bottom. The two stars indicate our data points 700 and 120 mJy at λ = 1.3 and 2.7 mm, respectively.

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