Constraining the gas mass of Herbig disks using CO isotopologues

Open Access

Fig. 13

Same as Fig. 8, but for ¹³C¹⁷O J = 2–1. The gray dashed line indicates a typical ALMA 3a detection of 1 mJy km s⁻¹ at a distance of 150 pc, which is achievable within an hour of integration time. The J = 3–2 transition can be found in Fig. C.2.

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