Table 1
Stellar properties of our sample.
| Star | SpT | Teff | L⋆ | M⋆ (a) | D (b) | ks (c) | Reference(s) |
|---|---|---|---|---|---|---|---|
| (K) | (L⊙) | (M⊙) | (pc) | ||||
| CQ Tau | F5 | 6750 ± 300 | 6.17 ± 2.12 | 1.49 ± 0.11 | 149.4 ± 1.3 | 1.43 | (1,2) |
| DoAr 44 | K2 | 5100 ± 150 | 0.87 ± 0.34 | 1.13 ± 0.16 | 146.3 ± 0.5 | 1.23 | (3) |
| GM Aur | K5 | 4440 ± 150 | 1.25 ± 0.32 | 0.97 ± 0.16 | 158.1 ± 1.2 | 1.11 | (3) |
| HD 100453 | A9 | 7250 ± 250 | 6.15 ± 1.07 | 1.59 ± 0.06 | 103.8 ± 0.2 | 1.51 | (4,5) |
| HD 100546 | A0 | 9750 ± 500 | 24.16 ± 5.99 | 2.13 ± 0.11 | 108.1 ± 0.4 | 1.63 | (5) |
| HD 135344 B | F8 | 6375 ± 125 | 6.54 ± 1.49 | 1.56 ± 0.11 | 135.0 ± 0.4 | 1.39 | (6,5) |
| HD 139614 | A9 | 7750 ± 250 | 5.97 ± 1.22 | 1.57 ± 0.06 | 133.6 ± 0.5 | 1.51 | (5) |
| HD 142527 | F6 | 6500 ± 250 | 10.18 ± 0.36 | 1.75 ± 0.10 | 159.3 ± 0.7 | 1.41 | (5) |
| HD 169142 | F1 | 10700 ± 850 | 20.58 ± 8.04 | 2.11 ± 0.14 | 114.9 ± 0.4 | 1.48 | (7,2) |
| HD 97048 | A0 | 10500 ± 50 | 36.56 ± 20.03 | 2.36 ± 0.19 | 184.4 ± 0.8 | 1.63 | (5) |
| IP Tau | M0 | 3850 ± 100 | 0.07 ± 0.00 | 0.59 ± 0.02 | 129.4 ± 0.3 | 0.96 | (8,9) |
| LkCa 15 | K2 | 5100 ± 150 | 1.51 ± 0.31 | 1.40 ± 0.11 | 157.2 ± 0.7 | 1.23 | (3) |
| LkHα 330 | G4 | 5680 ± 50 | 22.81 ± 0.62 | 3.05 ± 0.07 | 318.2 ± 3.5 | 1.33 | (3) |
| PDS 70 | K7 | 3972 ± 36 | 0.35 ± 0.09 | 0.76 ± 0.02 | 112.4 ± 0.2 | 1.02 | (10,11,12) |
| RX J1615 | K7 | 4100 ± 150 | 0.62 ± 0.18 | 0.73 ± 0.14 | 155.6 ± 0.6 | 1.02 | (3) |
| RY Lup | K2 | 5100 ± 150 | 1.72 ± 0.74 | 1.47 ± 0.21 | 153.5 ± 1.4 | 1.23 | (13,14) |
| SZ Cha | K2 | 5100 ± 150 | 1.65 ± 0.35 | 1.45 ± 0.11 | 190.2 ± 0.9 | 1.23 | (3) |
| UX Tau A | K2 | 5270 ± 100 | 1.62 ± 0.08 | 1.38 ± 0.05 | 142.2 ± 0.7 | 1.23 | (9) |
| V1247 Ori | F0 | 7875 ± 375 | 16.33 ± 6.23 | 1.88 ± 0.14 | 401.3 ± 3.2 | 1.49 | (5) |
| V1366 Ori | B9.5 | 9500 ± 250 | 10.37 ± 4.42 | 1.90 ± 0.06 | 308.6 ± 2.2 | 1.66 | (5) |
Notes. (a)The masses are derived from the effective temperatures and updated luminosities as detailed in Sect. 2.1. (b)Distances are derived from the parallax measurements provided by Gaia EDR3 (Gaia Collaboration 2021) as D = 1∕ϖ. (c)Stellar spectral index as defined in Eq. (B.3). Evaluated at λ0 = 2.25 μm.
References. (1) Mora et al. (2001); (2) Vioque et al. (2018); (3) Manara et al. (2014); (4) Vieira et al. (2003); (5) Fairlamb et al. (2015); (6) Coulson & Walther (1995); (7) Murphy et al. (2015); (8) Herbig et al. (1986); (9) Herczeg & Hillenbrand (2014); (10) Pecaut & Mamajek (2016); (11) Keppler et al. (2018); (12) Müller et al. (2018); (13) Gahm et al. (1989); (14) Alcalá et al. (2017).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.