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Table 3

Photospheric and best-fit/most-probable disk parameters from this work.

ID Teff L∗ AV Rin Mdisk (B) Mdisk (P) β (B) β (P) H100 (B) H100 (P) i
[K] [10-3L⊙] [mag] [AU] [10-5 M⊙] [10-5 M⊙] [AU] [AU] [°]
1 2400 0.355 ± 0.106 0.1 ± 0.01 0.004 1.0 1.0 1.10 1.10 20 20 60
2 2500 2.367 ± 0.336 0.1 ± 0.01 0.025 0.1 0.1 1.175 1.175 14 14 45
3 2100 6.139 ± 1.852 0.26 ± 0.26 0.038 3.16 1.0 1.10 1.10 16 16 15
4 2800 64.2 ± 10.49 3.6 ± 0.15 0.041 3.16 3.16 1.10 1.10 16 16 30
5 2800 23.18 ± 4.020 2.28 ± 0.18 0.025 10.0 10.0 1.10 1.125 20 18 30
6 2800 81.15 ± 12.94 7.2 ± 0.25 0.317 10.0 10.0 1.125 1.125 14 14 60
7 2600 379.1 ± 58.95 3.94 ± 0.98 0.015 0.1 0.32 1.15 1.15 20 20 15
8 1700 2.4 ± 0.54 2.6 ± 0.20 0.023 3.25 3.16 1.31 1.30 15.6 16 60
9 2800 5.459 ± 0.352 3.0 ± 0.19 0.038 3.16 3.16 1.20 1.175 8 10 15
10 2500 6.242 ± 0.325 4.8 ± 0.22 0.005 0.1 0.1 1.025 1.05 18 18 60
11 2600 3.54 ± 0.192 1.35 ± 0.1 0.005 1.0 0.32 1.10 1.10 8 10 30
12 2600 5.603 ± 0.376 1.41 ± 0.07 0.038 1.0 1.0 1.10 1.10 8 8 60
13 2200 1.221 ± 0.080 0.2 ± 0.03 – – – – – – – –
14 2400 3.22 ± 0.152 1.27 ± 0.07 – – – – – – – –
15 2500 5.591 ± 0.237 1.89 ± 0.1 – – – – – – – –
16 2600 4.078 ± 0.177 3.91 ± 0.23 0.010 100 100 1.10 1.075 20 20 45
17 2700 10.43 ± 0.429 1.71 ± 0.1 0.051 3.16 1.0 1.10 1.125 8 10 45
18 1800 3.045 ± 0.185 1.04 ± 0.1 – – – – – – – –
19 2500 3.749 ± 0.159 3.45 ± 0.18 – – – – – – – –
20 2400 4.044 ± 0.181 0.42 ± 0.42 0.008 100 100 1.137 1.125 21 20 45
21 2200 2.814 ± 0.165 0.57 ± 0.08 – – – – – – – –
22 2200 2.66 ± 0.165 0.39 ± 0.13 0.4 3.16 1.0 1.0 1.0 11 12 30
23 2700 18.74 ± 0.799 2.42 ± 0.17 – – – – – – – –
24 2400 2.517 ± 0.139 2.14 ± 0.16 0.4 31.6 31.6 1.05 1.05 20 18 60
25 2000 2.8 ± 0.140 0.0 ± 0.04 0.159 3.16 1.0 1.05 1.075 8 6 45
26 2400 3.564 ± 0.171 0.4 ± 0.1 – – – – – – – –
27 2300 2.862 ± 0.137 0.9 ± 0.1 – – – – – – – –
28 3000 1.459 ± 0.076 2.89 ± 0.16 0.008 3.16 0.32 1.0 1.025 11 12 30
29 2200 20.46 ± 0.884 0.56 ± 0.04 0.9 1.0 0.1 1.0 1.0 2 2 60
30 2300 5.669 ± 0.237 1.43 ± 0.07 0.013 3.16 3.162 1.05 1.025 11 8 45
31 2800 10.15 ± 0.612 0.95 ± 0.32 0.044 0.32 0.32 1.20 1.20 18 20 45
32 2800 47.78 ± 1.954 4.7 ± 0.36 0.0377 10.0 10.0 1.05 1.075 8 10 45
33 2800 82.84 ± 3.77 2.8 ± 0.2 0.126 10.0 10.0 1.125 1.125 4 4 45
34 2600 27.39 ± 0.995 15.0 0.051 316 316 1.175 1.175 20 20 45
35 2800 51.18 ± 2.105 5.42 ± 0.42 0.041 3.16 3.16 1.20 1.20 10 12 45
36 1900 17.52 ± 0.933 2.31 ± 0.33 0.051 10.0 3.16 1.025 1.05 12 12 45
37 3000 64.0 ± 2.775 3.58 ± 0.36 0.017 3.16 3.16 1.25 1.25 18 18 45
38 2200 30.73 ± 6.521 7.74 ± 0.48 0.025 0.32 1.0 1.10 1.125 18 18 60
39 2400 26.27 ± 5.909 2.3 ± 0.21 0.063 1.0 1.0 1.15 1.15 10 10 45
40 3000 43.82 ± 1.729 4.3 ± 0.29 0.015 0.1 0.1 1.05 1.025 4 4 30
41 2800 23.81 ± 1.39 1.16 ± 0.1 0.063 0.32 0.32 1.175 1.175 18 16 60
42 2800 28.93 ± 5.848 0.04 ± 0.01 0.025 10.0 10.0 1.075 1.075 18 14 60
43 2100 12.48 ± 2.211 1.93 ± 0.19 0.044 0.32 0.32 1.225 1.225 18 18 30
44 2400 16.49 ± 5.241 1.02 ± 0.26 0.018 1.0 1.0 1.225 1.225 20 18 30
45 2800 34.59 ± 7.973 1.0 ± 0.1 0.013 0.1 0.1 1.275 1.275 10 10 30
46 3000 13.02 ± 3.103 0.6 ± 0.1 0.021 0.32 0.32 1.175 1.175 12 12 60
47 2500 6.242 ± 1.354 1.3 ± 0.1 0.032 3.16 10.0 1.175 1.175 16 16 30
48 2900 30.6 ± 7.081 0.3 ± 0.1 0.012 1.0 1.0 1.15 1.15 14 14 45
49 3400 27.66 ± 6.102 3.38 ± 0.23 0.010 1.0 1.0 1.20 1.20 16 16 45
50 2800 10.34 ± 2.422 1.3 ± 0.1 0.007 31.6 31.6 1.125 1.15 18 18 30
51 2800 14.88 ± 3.411 1.5 ± 0.1 0.051 1.0 1.0 1.10 1.10 6 6 60
52 2600 26.31 ± 6.167 0.6 ± 0.1 0.01 0.32 0.32 1.20 1.225 10 10 45
53 2600 6.486 ± 1.574 0.7 ± 0.1 0.006 10.0 10.0 1.10 1.10 20 20 60
54 3000 42.35 ± 9.502 1.7 ± 0.1 0.014 0.3 0.32 1.20 1.20 8 8 30
55 3000 21.45 ± 4.865 1.5 ± 0.1 0.025 0.15 0.32 1.175 1.175 20 18 45

Notes. (1) We list the disk parameters for all objects in our sample with detected excess emission at IR wavelengths. (2) The error in Teff is 100 K for all cases except for object 8 (i.e., OTS 44) with a larger value of 140 K. (3) We fixed AV = 15 mag for object 34, see an explanation in Sect. 4.1. (4) The total disk mass Mdisk is calculated from the dust mass assuming a gas-to-dust mass ratio of 100. (5) The tags B and P quoted in brackets for Mdisk, β and H100 denote the best-fit and the most probable values, respectively. The values of the disk inner radius Rin and the inclination i are for the best-fit models.

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