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Table 3
Stellar parameters derived for the objects in our sample.
| Name | SpT | Teff [K] | log(L∗/L⊙) | M∗[M⊙] | ⟨log(Lacc,noise/L⊙)⟩ |
|
|
|||||
| TWA9A | K5 | 4350 | −0.61 | 0.81 | −3.38 |
| SO879 | K7 | 4060 | −0.29 | 1.07 | −2.88 |
| TWA6 | K7 | 4060 | −0.96 | 0.66 | −3.37 |
| TWA25 | M0 | 3850 | −0.61 | 0.84 | −3.04 |
| TWA14 | M0.5 | 3780 | −0.83 | 0.73 | −3.23 |
| TWA13B | M1 | 3705 | −0.70 | 0.68 | −3.32 |
| TWA13A | M1 | 3705 | −0.61 | 0.70 | −2.85 |
| TWA2A | M2 | 3560 | −0.48 | 0.55 | −3.36 |
| Sz122 | M2 | 3560 | −0.60 | 0.54 | −2.57 |
| TWA9B | M3 | 3415 | −1.17 | 0.37 | −3.93 |
| TWA15B | M3 | 3415 | −0.96 | 0.37 | −3.45 |
| TWA7 | M3 | 3415 | −1.14 | 0.37 | −3.84 |
| TWA15A | M3.5 | 3340 | −0.95 | 0.30 | −3.23 |
| Sz121 | M4 | 3270 | −0.34 | 0.37 | −3.25 |
| Sz94 | M4 | 3270 | −0.76 | 0.28 | −3.38 |
| SO797 | M4.5 | 3200 | −1.26 | 0.19 | −4.27 |
| SO641 | M5 | 3125 | −1.53 | 0.12 | −4.51 |
| Par−Lup3−2 | M5 | 3125 | −0.75 | 0.18 | −3.89 |
| SO925 | M5.5 | 3060 | −1.59 | 0.10 | −4.65 |
| SO999 | M5.5 | 3060 | −1.28 | 0.13 | −4.30 |
| Sz107 | M5.5 | 3060 | −0.79 | 0.16 | −3.69 |
| Par−Lup3−1 | M6.5 | 2935 | −1.18 | 0.10 | −4.74 |
| TWA26 | M9 | 2400 | −2.70 | 0.02 | −6.54 |
| TWA29 | M9.5 | 2330 | −2.81 | 0.02 | −6.64 |
Notes. The spectral type-Teff relation is adopted from Luhman et al. (2003) for M-type objects and from Kenyon & Hartmann (1995) for K-type objects.
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