Table 1
Properties of the sample.
| Name | d(a) | Teff(a) | log g(a) | logL*(a) | M*(a) | logLacc(a) | V(b) | Av(c) | K(d) | v sin i(e) | vrad(e) | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (pc) | (K) | (cm s-2) | (L⊙) | (M⊙) | (L⊙) | (mag) | (mag) | (mag) | (km s-1) | (km s-1) | ||
| [1] | HD 37806 | 428 | 10500 | 4.0 |  |
 |
 |
7. 9 | 0. 13 | 5. 6 |  |
47 |
| [2] | HD 38120 | 405 | 10700 | 4.0 |  |
 |
 |
9.1 | 0.21 | 7. 2 |  |
28 |
| [3] | HD 45677 | 620 | 16500 | 4.0 |  |
 |
 |
7. 4 | 0. 57 | 4. 5 | 200 | 22 |
| [4] | HD 58647 | 319 | 10500 | 3.3 |  |
 |
 |
6. 8 | 0. 37 | 5. 4 | 118 ± 4 | |
| [5] | HD 85567 | 1023 | 13000 | 3.5 |  |
 |
 |
8. 5 | 0. 89 | 5. 8 | 31 ± 3 | |
| [6] | HD 95881 | 1168 | 10000 | 3.2 |  |
 |
 |
8. 2 | 0. 72 | 5. 7 | 50 | 36 |
| [7] | HD 97048 | 185 | 10500 | 4.3 |  |
 |
 |
8. 4 | 0. 90 | 5. 9 | 140 ± 20 | 18 |
| [8] | HD 98922 | 689 | 10500 | 3.6 |  |
 |
 |
6. 7 | 0. 09 | 4. 4 | 50 ± 3 | 0 |
| [9] | HD 100546 | 110 | 9750 | 4.3 |  |
 |
 |
6. 7 | 0. 00 | 5. 7 | 60 ± 5 | 9 |
| [10] | HD 114981 | 705 | 16000 | 3.6 |  |
 |
 |
7. 2 | 0. 15 | 7. 4 | 239± 13 | -50 ± 11 |
| [11] | HD 135344B(★) | 136 | 6375 | 4.0 |  |
 |
 |
8. 7 | 0. 53 | 7. 6 | 82 ± 2 | 0 |
| [12] | HD 139614(★) | 135 | 7750 | 4.3 |  |
 |
 |
8. 4 | 0. 21 | 6. 7 | 24 ± 3 | 0±2 |
| [13] | HD 141569 | 111 | 9500 | 4.2 |  |
 |
 |
7. 1 | 0. 38 | 6. 6 | 228 ± 10 | -12±7 |
| [14] | HD 142527(★) | 157 | 6500 | 3.9 |  |
 |
 |
8. 3 | 0. 00 | 5. 0 | -3. 5 | |
| [15] | HD 142666(★) | 148 | 7500 | 4.0 |  |
 |
 |
8. 8 | 0. 95 | 6. 1 | 65 ± 3 | -7 ± 3 |
| [16] | HD 144432(★) | 155 | 7500 | 4.0 |  |
 |
 |
8. 2 | 0. 48 | 5. 9 | 79 ± 4 | -3 ± 3 |
| [17] | HD 144668(★) | 161 | 8500 | 3.7 |  |
 |
 |
7. 2 | 0. 87 | 4. 4 | 199 ± 11 | -10±8 |
| [18] | HD 145718(★) | 153 | 8000 | 4.4 |  |
 |
 |
8. 8 | 1. 23 | 6. 7 | 113±3 | -4±2 |
| [19] | HD 150193 | 151 | 9000 | 4.0 |  |
 |
 |
8. 8 | 1. 80 | 5. 3 | 108±5 | -5 ± 4 |
| [20] | HD 158643 | 123 | 9800 | 3.6 |  |
 |
 |
4. 8 | 0. 00 | 4. 3 | 256 | -11 |
| [21] | HD 163296 | 102 | 9250 | 4.3 |  |
 |
 |
6. 8 | 0. 37 | 4. 6 | 129±8 | -9 ± 6 |
| [22] | HD 169142(★) | 114 | 10700 | 4.0 |  |
 |
 |
8. 2 | 1. 02 | 6. 4 | 48 ± 2 | 0±2 |
| [23] | HD 179218 | 266 | 9500 | 3.9 |  |
 |
 |
7. 8 | 0. 33 | 5. 8 | 69 ± 3 | 15±2 |
| [24] | HD 190073 | 870 | 9750 | 3.4 |  |
 |
 |
7. 7 | 0. 20 | 5. 7 | 0–8 | 0 |
| [25] | HD259431 | 721 | 14000 | 4.3 |  |
 |
 |
8. 7 | 1. 11 | 5. 7 | 83 ± 11 | 26 ± 8 |
| [26] | V1818Ori(★) | 695 | 13000 |  |
 |
11. 0 | 3. 72 | 6. 0 | 46 ± 10 | 26 |
Notes. (a)Distance, effective temperature, surface gravity, stellar luminosity and mass, and accretion luminosity from Vioque et al. (2018); Wichittanakom et al. (2020).(b) Visual magnitude from CDS-Simbad. (c)Visual extinction from Vioque et al. (2018). (d)2MASS K-band magnitude. (e)v sin i and radial velocity from Miroshnichenko et al. (2001); Guimarães et al. (2006); Kharchenko et al. (2007); Montesinos et al. (2009); Alecian et al. (2013); Ilee et al. (2014). (★)Sources for which Brγ emission was not detected above 10% of the continuum.
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