Table 3
Best-fitting parameters, with their respective errors, obtained from our axisymmetric kinematic model.
| Global geometric | Global kinematic | K-band continuum | Brγ | χ2 | |||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| parameters | parameters | disk geometry | disk geometry | ||||||||||||
| Parameter | i | PA | Vrot | j | ac | al | EW | V/R | – | ||||||
| (°) | (°) | (km s−1) | – | (D⋆) | (D⋆) | (Å) | – | – | |||||||
| HD 23630 | 53 ± | 5 | 110 ± | 5 | 270 ± | 25 | −0.45 ± | 0.05 | 1.3 ± 1.0 | 7.0 ± | 1.0 | 5.80 ± | 0.8 | 1.02 | 5.86 |
| HD 23862 | 85 ± | 5 | 333 ± | 10 | 410 ± | 50 | −0.47 ± | 0.05 | 4.0* | 11.0 ± | 1.0 | 8.86 ± | 1.0 | 1.00 | 2.31 |
| HD 28497 | 44 ± | 10 | 30 ± | 10 | 600 ± | 50 | −0.35 ± | 0.05 | 6.0 ± 2.0 | 11.0 ± | 2.0 | 14.00 ± | 3.0 | 1.29 | 0.96 |
| HD 30076 | 38 ± | 5 | 73 ± | 4 | 400 ± | 20 | −0.45 ± | 0.05 | 6.0 ± 1.0 | 10.0 ± | 0.5 | 20.67 ± | 3.0 | 1.06 | 0.70 |
| HD 32991 | 40 ± | 10 | 157 ± | 5 | 500 ± | 50 | −0.50 ± | 0.05 | 2.0* | 13.0 ± | 2.0 | 20.00 ± | 2.0 | 1.07 | 0.62 |
| HD 35439 | 55 ± | 5 | 45 ± | 20 | 397 ± | 50 | −0.50 ± | 0.05 | 1.7* | 4.5 ± | 0.3 | 20.00 ± | 5.0 | 0.96 | 1.01 |
| HD 36576 | 60 ± | 5 | 198 ± | 10 | 380 ± | 50 | −0.40 ± | 0.02 | 2.0 ± 1.0 | 13.0 ± | 1.0 | 15.00 ± | 3.0 | 1.01 | 1.60 |
| HD 37202 | 67 ± | 5 | 127 ± | 5 | 400 ± | 30 | −0.45 ± | 0.03 | 4.7* | 4.8 ± | 0.4 | 7.43 ± | 2.0 | 1.02 | 3.19 |
| HD 37490 | 49 ± | 5 | 305 ± | 5 | 308 ± | 30 | −0.50 ± | 0.05 | 1.0* | 2.5 ± | 0.5 | 11.62 ± | 3.0 | 1.02 | 0.97 |
| HD 41335 | 68 ± | 5 | 55 ± | 5 | 400 ± | 30 | −0.60 ± | 0.03 | 2.0* | 5.0 ± | 0.4 | 17.00 ± | 4.0 | 0.95 | 1.98 |
| HD 45725 | 72 ± | 5 | 101 ± | 5 | 440 ± | 40 | −0.50 ± | 0.03 | 1.2* | 12.0 ± | 1.0 | 22.70 ± | 2.0 | 0.97 | 2.71 |
| HD 60606 | 70 ± | 10 | 240 ± | 10 | 390 ± | 20 | −0.50 ± | 0.05 | 2.0* | 7.5 ± | 0.5 | 17.00 ± | 2.0 | 1.03 | 1.23 |
| HD 66194 | 55 ± | 5 | 220 ± | 20 | 350 ± | 50 | −0.40* | 3.0* | 8.0 ± | 1.0 | 10.73 ± | 2.0 | 1.01 | 0.78 | |
| HD 68980 | 22 ± | 3 | 310 ± | 5 | 410 ± | 40 | −0.50 ± | 0.05 | 1.5* | 3.0 ± | 0.5 | 25.00 ± | 4.0 | 1.03 | 1.16 |
| HD 209409 | 70 ± | 5 | 290 ± | 5 | 355 ± | 50 | −0.45 ± | 0.03 | 3.0* | 8.0 ± | 0.5 | 18.12 ± | 2.0 | 1.02 | 2.50 |
| HD 212076 | 22 ± | 5 | 202 ± | 20 | 400 ± | 60 | −0.50 ± | 0.05 | 3.0* | 4.0 ± | 0.5 | 12.00 ± | 2.0 | 1.01 | 1.16 |
| HD 212571 | 34 ± | 10 | 87 ± | 15 | 440 ± | 40 | −0.50 ± | 0.1 | 1.5* | 2.0 ± | 0.3 | 6.00 ± | 2.0 | 1.00 | 1.01 |
| HD 214748 | 73 ± | 10 | 67 ± | 10 | 244 ± | 20 | −0.46 ± | 0.03 | 2.0* | 3.9 ± | 0.4 | 5.00 ± | 0.5 | 1.04 | 1.85 |
| HD 37795 | 35 ± | 5 | 10 | 350 ± | 10 | −0.5 ± | 0.1 | 2.0 ± 0.5 | 5.5 ± | 0.3 | 7.0 ± | 0.5 | 1.04 | 4.0 | |
| HD 50013 | 35 ± | 10 | 25 ± | 10 | 480 ± | 40 | −0.5 ± | 0.2 | 3.5 ± 0.5 | 6.2 ± | 2.0 | 13.0 ± | 2.0 | 1.13−1.10 | 6.8 |
| HD 89080 | 65 ± | 10 | 5 ± | 5 | 300 ± | 20 | −0.45 ± | 0.1 | 3.0 ± 1.0 | 6.5 ± | 1.0 | 5.8 ± | 0.5 | 1.04 | 1.1 |
| HD 91465 | 70 ± | 10 | −25 ± | 10 | 400 ± | 30 | −0.45 ± | 0.1 | 2.0 ± 0.5 | 11.0 ± | 2.0 | 10.0 ± | 1.0 | <1 | 2.5 |
| HD 105435 | 35 ± | 15 | 40 ± | 10 | 500 ± | 50 | −0.5 ± | 0.3 | 2.0 ± 1.0 | 9.0 ± | 2.0 | 19.2 ± | 2.0 | ~1 | 2.3 |
| HD 120324 | 25 ± | 5 | 80 ± | 15 | 510 ± | 20 | −0.5 ± | 0.1 | <3.0 | 4.0 ± | 1.0 | 5.6 ± | 0.3 | 1.03 | 1.3 |
| HD 158427 | 45 ± | 5 | 88 ± | 2 | 480 ± | 20 | −0.5 ± | 0.1 | <2.0 | 5.8 ± | 0.5 | 14.5 ± | 1.0 | 1.01 | 1.7 |
Notes. In the case of HD 28497 we modified the used model to include a spiral above the Gaussian distribution (see Sect. 4.3). Upperrows correspond to the disk parameters determined in this work, and the lower rows show the values from Meilland et al. (2012).
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