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Table 1

Stellar properties used in this study.

Source Class Mass L EW(Hα) log (Ṁ⊙ yr-1) LX Lmid − IR log(L [O   I] /L⊙) Jeta Ref.
(M⊙) (L⊙) (Å) (1030 erg/s) (1032 erg/s)
AA Tau II 0.76 0.80 37 –8.48 1.24 1.27 –4.68 √ 1, 22, 25
BP Tau II 0.75 0.95 40 –7.88 1.36 1.80 –4.77  ×  1, 22
CW Tau II 1.40 1.10 135 –7.99 2.84 4.62 –2.43 √ 1, 23, 26
CZ Tau (A, B) III 0.32 0.27 4 –9.35 2.24 3.11 ...  ×  1, 2
DF Tau (A, B) II 0.34 1.77 54 –7.96 ... 2.62 –3.81 √ 2, 3, 26
DG Tau I/II 0.91 1.70 63 –6.13 0.55 15.8 –2.71 √ 1, 4, 7, 22, 27
DG Tau B I/II 0.72 5.50 276 ... 9.69 5.09 ... √ 1, 31
DK Tau II 0.74 1.30 40 –7.42 0.92 3.93 –3.85  ×  1, 22
DL Tau II 0.75 0.85 105 –7.17 ... 2.87 –4.26 √ 1, 2, 5, 25
DM Tau II 0.47 0.30 139 –8.67 3.18 0.30 ...  ×  1, 5
DN Tau II 0.56 1.00 20 –8.72 1.15 1.19  <  −5.18  ×  1, 2, 22
DO Tau II 0.70 1.05 100 –7.52 0.18 7.56 –3.97 √ 3, 6, 7, 22, 25
DR Tau II 0.75 0.96 106 –7.49 ... 7.41 –3.91 √ 2, 3, 6, 22, 25
FS Tau A II 0.53 0.15 81 –9.50 3.22 3.24 ...  ×  1, 6
FV Tau (A, B) II 0.88 0.98 50 –6.23 0.53 5.93 ...  ×  1
FX Tau II 0.47 1.02 10–15 –8.65 0.50 1.27 –4.85  ×  1, 22
FZ Tau II 0.57 0.98 181 –7.69 0.64 2.81 ...  ×  1, 2
GG Tau II 0.44 0.98 30 –7.76 ... 2.50 –4.57  ×  3
GI Tau II 0.75 1.00 20 –8.08 0.83 3.57 –4.46  ×  1, 23
GK Tau (A, B) II 0.74 1.40 25 –8.19 1.47 3.80 –4.36  ×  1, 22
GV Tau (A, B) I 0.68 1.82 86 –6.71 0.65 64.7 ...  ×  1
HL Tau I 1.20 1.53 49 –6.80 3.84 29.7 –3.59 √ 1, 22, 25
HN Tau II 1.10 0.25 150 –8.60 0.15 2.67 –3.46 √ 1, 2, 23, 25
HP Tau II 1.39 1.40 28 ... 2.55 3.63 ... √ 1, 27
HQ Tau III ... ... 2 ... 8.16 3.75 ...  ×  1, 8
IQ Tau II 0.51 0.88 13 –7.55 0.42 1.43 ...  ×  1
RY Tau II 2.37 7.60 13 –7.04 5.52 35.8 –3.65 √ 1, 22
T Tau II 2.41 8.90 41 –7.24 8.05 59.5 –2.63 √ 1, 22, 27
UX Tau A II 1.10 1.81 9.5 –9.30 0.95 1.27  <  − 4.97  ×  2, 6, 9, 22
UZ Tau II 0.47 0.49 73 –8.01 0.89 3.98 ...  ×  1
VY Tau III 0.57 0.55 4.9 ... 1.29 0.38  <  − 5.56  ×  2, 7, 10, 22
XZ Tau (A, B) II 0.34 0.33 62 –8.74 0.96 13.1 ... √ 1, 2, 25
Coku Tau-1 II 0.70 0.15 70 –7.36 ... 3.90 ... √ 1, 31
Coku Tau-3 II 0.46 0.98 5 ... 5.85 1.31 ...  ×  1
Coku Tau-4 II 0.43 0.68 1.8 ...  < 0.21 0.70 ...  ×  2, 9, 10
AB Aur HAe 2.40 49.00 33 –6.85 0.35 64.6 –3.36 √ 1, 11, 28
GM Aur II 0.52 0.74 96 –8.02 1.68 0.68 –4.90  ×  3, 5, 7, 22
RW Aur A II 1.34 3.37 76 –7.50 1.60 4.70 –3.11 √ 4, 23, 25, 32
SU Aur II 1.91 9.90 63 –8.20 9.46 15.0  <  − 3.85  ×  1, 22
UY Aur (A, B) II 0.57 1.25 36 –7.37  < 0.25 10.6 –3.62 √ 2, 9, 12, 23, 25
Haro 6-28 II 0.21 0.12 48–92 –8.10 0.25 0.47 ...  ×  1, 12
Haro 6-37 II 0.91 1.74 22 –8.12 ... 2.35  <  − 5.07  ×  2, 6, 22
L1551 IRS5 I 1.58 2.60 83 –6.47 0.021 62.0 ... √ 1, 13, 14, 30
MHO-1/2 I/II 0.34 0.42 58  <  −8.48 1.64 7.20 ...  ×  1
V710 Tau II 0.68 1.10 69 ... 1.38 0.75 ...  ×  1, 6
V773 Tau II 0.58 5.60 2  <  −8.6 9.49 4.46 –3.93  ×  1, 6, 22
V892 Tau HAe 2.89 77.00 7–13 ... 9.21 132 ... √ 1, 29
HBC 366 III 0.40 2.60 1.3  <  − 8.94 4.14 0.23 ...  ×  1, 16
HD 31648 HAe 2.30 23.7 18.3 –8.39 ... 34.8 ...  ×  17
HD 35187 HAe 2.30 1.37 5.1 –7.81 ... 18.5 ... √ 11, 18
HD 36112 HAe 2.20 1.45 14.5 –6.70 ... 17.4 ...  ×  18, 19
IC2087IR II ... ... 22 –6.20 4.67 16.3 ...  ×  1
IRAS 04016+2610 I 1.45 3.70 41–56 –7.15 4.47 13.6 ... √ 1, 21, 27
IRAS 04101+3103 HAe ... ... 11 ... ... 10.7 ...  ×  15
IRAS 04108+2803 B I 0.36 0.4 ... ... 0.42 2.46 ... √ 1, 27
IRAS 04239+2436 I ... 1.27 ... ... ... 8.76 ... √ 13, 27
IRAS 04278+2253 I ... 7.20 17 –5.18 ... 28.6 ...  ×  4, 20, 21
IRAS 04299+2915 II ... ... 6.5 ... ... 0.47 ...  ×  15
IRAS 04303+2240 II 0.51 2.20 67 –6.05 5.01 6.43 ...  ×  1
IRAS 04361+2547 I ... 3.70 ... ...  < 0.30 8.28 ... √ 1, 9, 27
IRAS 04365+2535 I ... 2.20 ... ... 1.99 6.13 ... √ 1, 27
SST 041412.2+280837 I ... ... ... ... ... 1.73 ...  ×  33
SST 042936.0+243555 II ... ... ... ... ... 0.32 ...  ×  24, 33
SST 043905.2+233745 I/II ... ... ... ... ... 0.23 ...  ×  24, 33

Notes. 

(a)

√ indicates presence of jet,  ×  indicates that no jet has been reported.

(b)

“...” indicates no information available.

References. 1 Güdel et al. (2007); 2 Watson et al. (2009); 3 Gullbring et al. (1998); 4 White & Hillenbrand (2004); 5 Herbig & Bell (1995); 6 White & Ghez (2001); 7 Güdel priv. comm. 2009; 8 Nguyen et al. (2009); 9 Neuhäuser et al. (1995); 10 Cohen & Kuhi (1979); 11 Garcia Lopez et al. (2006); 12 compiled in McCabe et al. (2006); 13 Prato et al. (2009); 14 Kenyon et al. (1998); 15 Kenyon et al. (1990); 16 compiled in Martin et al. (1994); 17 Mannings & Sargent (1997); 18 Manoj et al. (2006); 19 Isella et al. (2008); 20 Bitner et al. (2008); 21 Furlan et al. (2008); 22 Cabrit et al. (1990); 23 Hartigan et al. (1995); 24 Luhman et al. (2010); 25 Hirth et al. (1997); 26 Hartigan et al. (2004); 27 Moriarty-Schieven et al. (1992); 28 Corcoran & Ray (1997); 29 Maheswar et al. (2002); 30 Davis et al. (2003); 31 Eislöffel & Mundt (1998); 32 Güdel et al. (2010); 33 Rebull et al. (2010).

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