Table 1
Stellar properties of the sources in the sample.
| Star | Sp. type | Teff | AV | Lstar/L⊙ | Mstar/M⊙ | log t ± σlog t (t in yr) | Ref.3 | ||
|
|
|||||||||
| BP Tau | K7 | 4060 | 0.49 |
|
0.78 ± 0.08 | 6.51 ± 0.12 | 1 | ||
| CI Tau | K7 | 4060 | 1.77 |
|
0.76 ± 0.08 | 6.27 ± 0.28 | 1 | ||
| CQ Tau | A8/F2 | 7200 | .. | 12 |
1.7 | 6.7 | 2 | ||
| CY Tau | M1 | 3720 | 0.1 | 0.4  |
0.48 ± 0.05 | 6.37 ± 0.11 | 1 | ||
| DG Tau | K7-M0 | 4000 | ... | 6.36 | 0.7 | 5.45 ± 0.15 | 3 | ||
| DL Tau | K7 | 4060 | ... | 1.12 | 0.7 | 6.23 ± 0.15 | 3 | ||
| DM Tau | M1 | 3720 | 0 |
|
0.47 ± 0.06 | 6.87 ± 0.34 | 1 | ||
| DQ Tau | M0 | 3850 | 0.97 | 0.91 | 0.55 | 6.00 ± 0.15 | 3 | ||
| FT Tau | C | < 5000 | 0.38 | [0.7,1.0 ] | > 6.0 | 3, this work | |||
| GM Aur | K3 | 4730 | 0.14 |
|
1.37 ± 0.17 | 6.87 ± 0.23 | 1 | ||
| LkCa 15 | K5 | 4350 | 0.62 |
|
1.12 ± 0.08 | 6.7 ± 0.16 | 1 | ||
| MWC 480 | A4 | 8460 | 11.5 | 1.8 | 6.7 | 4 | |||
| MWC 758 | A3 | 11 | 1.8 | 6.7 | 2 | ||||
| UZ Tau E | M1 | 3720 | 1.49 | > 0.88 | 0.5 | 6.20 ± 0.15 | 3 | ||
| UZ Tau W | M3 | 3470 | 0.83 | > 0.38 | 0.35 | 6.20 ± 0.15 | 3 | ||
| HL Tau | K7 | 4060 | ... | 6.60 | 0.7 | 5.45 ± 0.15 | 3 | ||
| HH 30 | M2-M3 | 3500 | ... | [0.2,0.9 ] | 0.25 | 6.2 ± 0.2 | 5 | ||
| DG Tau b | > 0.02 | 3 | |||||||
| T Tau N | K0 | 5250 | 1.39 | 15.5 | 1.9 | 6.70 ± 0.15 | 3 | ||
| Haro 6-10 a/b | K3 | 4800 | [1.8,3.3 ] | 1.5-1.8 | 6.3 ± 0.2 | 6 | |||
| Haro 6-13 | M0 | 3850 | .. | 2.1 | 0.55 | 5.70 ± 0.15 | 7 | ||
| Haro 6-33 | M0.5 | 3850 | .. | 0.76 | 0.55 | 6.17 ± 0.15 | 7 | ||
References. References for observational properties: (1) Bertout et al. (2007); (2) Chapillon et al. (2008); (3) Kenyon & Hartmann (1995); (4) Piétu et al. (2007); (5) Guilloteau et al. (2008); Pety et al. (2006); (6) Prato et al. (2009); (7) Schaefer et al. (2009). Note that ages have been derived homogeneously, using the Siess et al. (2000) tracks, but do not necessarily correspond to values cited in the other papers.
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