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The First Detection of ¹³C¹⁷O in a Protoplanetary Disk: A Robust Tracer of Disk Gas Mass

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Figure

Figure 1. (frequency of the hypera) The 1.25 mm continuum image from Isella et al. (2018)
Figure 2. Disk physical structure from Qi et al.of the CO snow line in both modelsModel 1T (2011)
Figure 3. ((modeled0.31a)–(e)) The deprojected and azimuthally averaged radial profiles of the observed and modeled CO lines
Figure 4. Toomre Q parameter for the new disk mass we derive in Model 2 andextrapolated back to 0.1 Myr

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