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Table 2

Parameters used in the disk models.

Source Model Teff R* Rin Tin Rgap Tgap H/Rout H/Rin Σdust,in PH/R Mdisk Notes
# (K) R (au) (K) (au) (K) (out/min) (out/min) (g cm−2) (in, out) (M)
RECX-5 #1 3350 0.76 0.018 1480* 1* 200 0.06/0.005 0.04/0.01 1e-5 1/7, 1/7 1.8e-3 Schmidt Nr = 10, pΣdust,in = −1.4, Small grains
RECX-9 #1 3305 0.95 0.02* 1500 0.07/0.005 1/7 1.4e-4
#2 0.07 830* 12 63 0.1/0.005 0.3/0.05 1e-5 1/7, 1/7 1.2e-4
#3 0.07 830* 20* 50 0.2/0.005 0.2/0.05 1e-5 1/7, 1/7 1.4e-4
RECX-11 #1 0.05 1500* 0.64 430* 0.08 0.12 2e-5 1/7, 1/7 2.5e-4
#2 0.05 1500* 0.64 430* 0.05 0.14 5e-5 1/7, 1/7 3.4e-4
#3 0.05 1500* 0.64 430* 0.05 0.14 5e-5 1/7, 1/7 3.4e-4 Small grains in inner disk
#4 0.05 1500* 0.64 430* 5e-5 3.4e-4 Well-mixed gas and dust
J0801 #1 3280 0.62 0.02 1250* 12.5 50* 0.03 0.03 1e-5 1/7, 1/7 le-4
#2 0.02 1250* 12.5 50* 0.03 0.03 1e-6 1/7, 1/7 8e-4
#3 0.02 1250* 19.5 40* 0.02 0.03 1e-6 1/7, 1/7 8e-4
#4 0.02 1250* 19.5 40* 0.01 0.01 1e-6 1/7, 1/7 8e-4
J0820 #1 3280 0.60 0.03 1000* 3 100* 0.17 0.05 1e-4 1/7, 1/7 4e-4
#2 0.03 1000* 2.1 120* 0.17 0.05 1e-4 1/7, 1/7 4e-4
#3 0.03 1000* 3 100* 0.05 0.20 1e-4 1/7, 1/7 4e-4
J0841 #1 0.03 900* 0.1* 495 0.04/0.005 0.1/0.05 1e-5 1/7, 1/7 1.2e-4
#2 0.03 900* 0.1* 495 0.03/0.005 0.1/0.05 1e-5 1/7, 1/7 4e-5
#3 0.03 900* 0.1* 495 0.03/0.005 0.1/0.05 1e-5 1/7, 0 8e-5
#4 0.03 900* 1.5* 130 0.02/0.005 0.1/0.01 3e-5 0, 0 5e-4
J0843 #1 3430 0.79 0.03 1200* 0.18* 495 0.28 0.17 5e-3 1/7, 1/7 3e-4 Small grains in inner disk
#2 0.03 1200* 0.9* 220 0.25 0.17 5e-3 1/7, 1/7 2.4e-4 Small grains in inner disk
J0844 #1 3145 0.37 0.03 750* 3* 78 1e-4 3.9e-4 Well-mixed gas and dust
#2 0.03 750* 2* 92 0.15 0.2 1e-4 1/7, 0 3.9e-4
#3 0.03 750* 3* 78 0.17 0.1 1e-4 1/7, 0 3.4e-4
#4 0.03 750* 3* 78 0.15 0.1 1e-4 1/7, 0 3.9e-4
η Cha #1 10500 2 1.6* 900 0.01/0.002 0 1.5e-6 Large grains, not flared, 100 au
#2 0.6* 1500 0.06/0.002 1/7 3e-7 Large grains
#3 0.9* 1200 0.03/0.002 1/7 3e-7 Large grains
#4 0.6* 1500 0.06/0.002 1/7 3e-7 Large grains, 50 au. Surface density power law pΣdust = −1.2

Notes. Rgap and Tgap refer to the location of a radial discontinuity, which may involve a thin gap and a change in radial properties (e.g., dust grain properties, vertical scale height, density power law). For some models we set the inner disk temperature in RADMC, and the distance is calculated accordingly, although the opposite is also feasible. In this table we list the distances as well because they are easier to compare with resolved observations and other models in the literature; the derived quantities are flagged with an asterisk (*). The parameter pH/R corresponds to the exponent in (H/R) ∝ Rp, and pΣdust,in is the power law vs. radius for the surface density in the inner disk. The notes include any further deviation from the standard model (see text) not reflected in the previous parameters.

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