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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 9.

Toomre Q parameter along radius in HL Tau. The dotted lines indicate the region when assuming a factor-of-two uncertainty in the disk mass mainly induced by κ 0 uncertainty (Ossenkopf & Henning 1994). Note that the Q value is smaller than or very close to 1.5 between 50 and 100 AU, which suggests that the region may be gravitationally unstable.

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