Table 3
Stellar, disk, and accretion parameters of the targets.
Name | dist | R in | SpT | T eff | A V | L ⋆ | log Lacc | M ⋆ | log Ṁacc | R ⋆ | Disk | Ref | |
[pc] | [AU] | [K] | [mag] | [ L⊙] | [ L⊙] | [ M⊙] | [ M⊙ yr-1] | [R⊙] | type | ||||
|
|||||||||||||
LkHα330 | 250 | 68 | G4 | 5800 | 3.0 | 14.40 | −0.6 | 2.35 ± 0.57 | −7.8 | 3.74 ± 1.08 | PTD | 1 | D |
DM Tau | 140 | 19 | M2 | 3560 | 1.1 | 0.36 | −1.3 | 0.56 ± 0.08 | −8.2 | 1.57 ± 0.46 | TD | 1 | B |
LkCa 15 | 140 | 50 | K2 | 4900 | 1.2 | 1.21 | −1.1 | 1.24 ± 0.33 | −8.4 | 1.52 ± 0.44 | PTD | 1 | B |
GM Aur | 140 | 28 | K5 | 4350 | 0.6 | 0.99 | −1.0 | 1.36 ± 0.36 | −8.3 | 1.75 ± 0.51 | PTD | 1 | B |
Sz-Cha | 160 | 29 | K2 | 4900 | 1.3 | 1.17 | −0.5 | 1.22 ± 0.32 | −7.8 | 1.50 ± 0.43 | PTD | 2 | B |
TW Hya | 55 | 4 | K7 | 4060 | 0.0 | 0.18 | −1.6 | 0.79 ± 0.17 | −8.9 | 0.85 ± 0.25 | TD | 3 | B |
CS Cha | 160 | 43 | K2 | 4900 | 0.8 | 1.45 | −1.0 | 1.32 ± 0.37 | −8.3 | 1.66 ± 0.48 | TD | 4 | B |
CHXR22E | 160 | 7 | M4 | 3270 | 2.6 | 0.07 | −4.1 | 0.24 ± 0.06 | −10.9 | 0.82 ± 0.24 | PTD | 2 | B |
Sz18 | 160 | 8 | M2 | 3560 | 1.3 | 0.26 | −1.9 | 0.54 ± 0.08 | −8.9 | 1.34 ± 0.39 | TD | 2 | B |
Sz27 | 160 | 15 | K7 | 4060 | 2.9 | 0.33 | −1.6 | 0.96 ± 0.24 | −8.9 | 1.16 ± 0.34 | PTD | 2 | B |
Sz45 | 160 | 18 | M0.5 | 3780 | 0.7 | 0.42 | −1.2 | 0.85 ± 0.11 | −8.3 | 1.51 ± 0.44 | TD | 2 | B |
Sz84 | 150 | 55 | M5 | 3125 | 0.5 | 0.24 | −2.3 | 0.24 ± 0.06 | −8.9 | 1.67 ± 0.49 | TD | 5 | B |
RX J1615 | 185 | 30 | K7 | 4060 | 0.0 | 0.89 | −1.3 | 1.16 ± 0.16 | −8.5 | 1.90 ± 0.55 | TD | 1 | B |
Oph 22 | 125 | 1 | M3 | 3415 | 3.0 | 0.56 | −2.9 | 0.53 ± 0.14 | −9.7 | 2.13 ± 0.62 | TD | 5 | B |
Oph 24 | 125 | 3 | M0 | 3850 | 4.0 | 0.42 | −2.0 | 0.92 ± 0.13 | −9.2 | 1.45 ± 0.42 | TD | 5 | B |
SR 21 | 125 | 36 | G4 | 5800 | 6.0 | 8.11 | −0.7a | 1.95 ± 0.50 | −7.9a | 2.81 ± 0.81 | PTD | 1 | D |
ISO-Oph196 | 125 | 15 | M5.5 | 3060 | 3.0 | 0.08 | −2.3 | 0.14 ± 0.04 | −8.9 | 1.00 ± 0.29 | PTD | 1 | B |
DoAr 44 | 125 | 30 | K2 | 4900 | 1.7 | 0.64 | −0.9 | 0.97 ± 0.19 | −8.2 | 1.11 ± 0.32 | PTD | 1 | B |
Ser 29 | 230 | 8 | M2 | 3560 | 2.6 | 0.04 | <−3.8 | 0.47 ± 0.08 | <−11.2 | 0.52 ± 0.15 | TD | 5 | B |
Ser 34 | 230 | 25 | M1 | 3705 | 2.7 | 0.26 | −2.7 | 0.71 ± 0.08 | −9.8 | 1.23 ± 0.36 | TD | 5 | B |
RX J1842.9 | 130 | 5 | K2 | 4900 | 0.4 | 0.56 | −1.5 | 0.93 ± 0.16 | −8.8 | 1.03 ± 0.30 | PTD | 6 | B |
RX J1852.3 | 130 | 16 | K2 | 4900 | 1.0 | 0.77 | −1.4 | 1.04 ± 0.19 | −8.7 | 1.21 ± 0.35 | TD | 6 | B |
Reference. For Rin: (1) Andrews et al. (2011); (2) Kim et al. (2009); (3) Hughes et al. (2007); (4) Espaillat et al. (2013); (5) Merín et al. (2010); (6) Hughes et al. (2010), evolutionary models used to derive M* and Ṁacc: (B) Baraffe et al. (1998), (D) D’Antona & Mazzitelli (1994). a Highly uncertain value.
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