Table B.2.
Stellar properties of our sample.
| Identifier | Teff | υ sin i | Radius | Mass | Rrad.core | log(τc) | Type | References for accretion type |
|---|---|---|---|---|---|---|---|---|
| (K) | (km s−1) | (R⊙) | (M⊙) | (R⊙) | (s) | |||
| BN Ori | 7020 ± 450 | 214 ± 24 |  |
 |
 |
 |
||
| CHX 22 | 5260 ± 200 | 9.87 ± 0.14 |  |
 |
 |
 |
wTTS | Spangler et al. (2001) |
| CO Ori | 6290 ± 220 | 69 ± 6 |  |
 |
 |
 |
cTTS | Astraatmadja & Bailer-Jones (2016) |
| COUP 1350 | 5590 ± 130 | 61.8 ± 1.0 |  |
 |
 |
 |
||
| CPD–43 7188 | 5360 ± 120 | 25.4 ± 0.5 |  |
 |
 |
 |
||
| CQ Tau | 6800 ± 290 | 94 ± 6 |  |
 |
 |
 |
||
| CR Cha | 4800 ± 230 | 34.5 |  |
 |
 |
 |
cTTS | Hussain et al. (2009) |
| GW Ori | 5700 ± 150 | 46.0 ± 1.6 |  |
 |
 |
 |
cTTS | Astraatmadja & Bailer-Jones (2016) |
| HBC 741 | 5470 ± 70 | 40.0 ± 0.8 |  |
 |
 |
 |
cTTS | Ducourant et al. (2005) |
| HD 133938 | 5290 ± 110 | 20.40 ± 0.23 |  |
 |
 |
 |
wTTS | Xing (2010) |
| HD 135127 | 6740 ± 120 | 108 ± 5 |  |
 |
 |
 |
wTTS | Krautter et al. (1997) |
| HD 137059 | 5840 ± 70 | 27.9 ± 1.7 |  |
 |
 |
 |
wTTS | Xing (2010) |
| HD 143978 | 6010 ± 120 | 36.1 ± 0.8 |  |
 |
 |
 |
wTTS | Xing (2010) |
| HD 147048 | 5410 ± 120 | 21.54 ± 0.41 |  |
 |
 |
 |
||
| IRAS 22144 + 6923 | 5720 ± 90 | 34.9 ± 1.0 |  |
 |
 |
 |
||
| IRAS 22152 + 6947 | 6620 ± 130 | 43.7 ± 2.4 |  |
 |
 |
 |
||
| NGC 2264 108 | 6130 ± 200 | 52.6 ± 1.8 |  |
 |
 |
 |
cTTS | Sousa et al. (2016) |
| NGC 2264 121 | 5450 ± 260 | 144 ± 12 |  |
 |
 |
 |
||
| NGC 2264 84 | 6160 ± 140 | 36.3 ± 0.7 |  |
 |
 |
 |
cTTS | Sousa et al. (2016) |
| NGC 6530 SCB 7 | 5490 ± 70 | 5.00 ± 0.22 | ||||||
| NGC 6530 SCB 739 | 6400 ± 100 | 4.28 ± 0.42 | ||||||
| PAR 102 | 6160 ± 100 | 49.3 ± 1.5 |  |
 |
 |
 |
||
| PAR 1391 | 6350 ± 160 | 14.99 ± 0.47 |  |
 |
 |
 |
||
| PAR 1394 | 6260 ± 140 | 62.9 ± 1.7 |  |
 |
 |
 |
||
| PAR 1414 | 5920 ± 120 | 33.9 ± 1.0 |  |
 |
 |
 |
||
| PAR 1455 | 5890 ± 120 | 23.5 ± 0.6 |  |
 |
 |
 |
||
| PAR 1646 | 6310 ± 80 | 15.67 ± 0.39 |  |
 |
 |
 |
||
| PAR 1736 | 6180 ± 110 | 55.3 ± 2.6 |  |
 |
 |
 |
||
| PAR 2441 | 5780 ± 110 | 13.40 ± 0.39 |  |
 |
 |
 |
||
| PX Vul | 7860 ± 410 | 81 ± 5 |  |
 |
 |
 |
||
| RY Ori | 6120 ± 110 | 49.7 ± 1.7 |  |
 |
 |
 |
cTTS | Richards et al. (2012) |
| V 1000 Sco | 4830 ± 200 | 25.8 ± 1.9 |  |
 |
 |
 |
wTTS | Luhman & Mamajek (2012) |
| V 1001 Sco | 5180 ± 130 | 24.6 ± 0.8 |  |
 |
 |
 |
wTTS | Luhman & Mamajek (2012) |
| V 1002 Sco | 4950 ± 220 | 76.7 ± 3.3 |  |
 |
 |
 |
||
| V 1044 Ori | 5500 ± 140 | 26.7 ± 0.8 |  |
 |
 |
 |
cTTS | Da Rio et al. (2009) |
| V 1149 Sco | 5740 ± 90 | 12.06 ± 0.23 |  |
 |
 |
 |
cTTS | Luhman & Mamajek (2012) |
| V 1152 Sco | 4800 ± 120 | 13.1 ± 0.7 |  |
 |
 |
 |
wTTS | Prugniel et al. (2011) |
| V 1156 Sco | 4820 ± 180 | 48.3 ± 3.2 |  |
 |
 |
 |
Notes. Columns are: effective temperature, projected rotational velocity, total radius of the star, mass, radius of the radiative core, convective turnover time at Hp/2 (at half a pressure scale height above the base of the convection zone), and accretion type. Error bars on Teff and υ sin i are detailled in Sect. 3.1.1, and error bars on the other parameters come from interpolations of the CESAM grids.
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