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Table 3

Mean line luminosities.

Star Nspectra d  ⟨ L ⟩   ⟨ L ⟩   ⟨ L ⟩   ⟨ L ⟩   ⟨ L ⟩ 
Hα [O i]6300 He i5876 Na iD2 Na iD1
(pc) (×1031 erg s-1) (×1029 erg s-1) (×1030 erg s-1) (×1030 erg s-1) (×1030 erg s-1)
HD 31648 3 146 10.4 [0.15] ... 2.35 [0.45] 3.91 [0.21] 3.86 [0.15]
HD 34282 2 1641 0.50  ±  0.08 ... 0.195 [0.27] 0.100 [0.36] 0.0644 [0.50]
HD 34700 1 3364 2.0  ±  0.3 ... ... 0.7  ±  0.2 0.6  ±  0.2
HD 58647 1 543 179  ±  10 81  ±  30 22  ±  9 31  ±  4 26  ±  4
HD 141569 4 991 2.51  ±  0.09 6  ±  1 ... 0.47  ±  0.05 0.481 [0.47]
HD 142666 3 1451 0.81  ±  0.08 ... 0.37  ±  0.07 0.470 [0.15] 0.40  ±  0.04
HD 144432 3 1451 4.79 [0.11] 0.4∗  ±  0.4 0.860 [0.53] 0.928 [0.68] 1.0  ±  0.1
HD 150193 2 203 6.2  ±  0.3 ... 0.9  ±  0.2 1.4  ±  0.2 1.1  ±  0.2
HD 163296 3 130 21.3 [0.05] 1.50∗ [1.73] 5.68 [0.41] 2.96 [0.39] 3.13 [0.48]
HD 179218 1 201 18  ±  1 4  ±  1 0.7  ±  0.2 0.6  ±  0.1 0.3  ±  0.1
HD 190073 1 767 360  ±  12 82  ±  10 68  ±  10 146  ±  10 128  ±  10
VX Cas 6 619 4.88 [0.18] 3.83 [0.16] 1.69 [0.62] 1.11 [0.41] 1.02 [0.40]
BH Cep 7 4501 1.26 [0.16] 0.784 [0.60] 0.537 [0.61] 0.669 [0.38] 0.578 [0.53]
BO Cep 5 4001 1.11 [0.24] 2.6  ±  0.5 0.464 [0.55] 0.277 [0.51] 0.232 [0.46]
SV Cep 5 596 6.52 [0.08] 7  ±  1 2.46 [0.41] 1.48 [0.49] 1.21 [0.42]
V1686 Cyg 6 9801 6.19 [0.44] 7.85 [0.35] (0.471 [0.90]) 2.64 [0.81] 1.47 [0.97]
VY Mon 1 8001 8.2  ±  0.2 39  ±  4 ... 1.5  ±  0.1 1.02  ±  0.08
51 Oph 3 142 23  ±  2 ... 8  ±  2 2.49∗ [1.06] 8  ±  2
KK Oph 3 1601 1.03  ±  0.03 3.54 [0.09] (0.0630 [0.42]) (0.0227 [0.31]) (0.0282 [0.28])
T Ori 3 472 12.6 [0.13] 7.49 [0.27] 1.972 [0.22] 2.18 [0.30] 1.52 [0.34]
BF Ori 4 603 14.8  ±  0.6 8  ±  1 9.86 [0.57] 9.66 [0.49] 9.38 [0.23]
CO Ori 5 4501 5.27 [0.07] 6.58 [0.22] 0.0573∗ [2.24] 0.469 [0.94] 0.397 [0.72]
HK Ori 5 4601 9.98 [0.41] 23.9 [0.4] 0.590∗ [0.68] (0.565 [0.20]) (0.566 [0.27])
NV Ori 5 4502 3.5  ±  0.2 0.457∗ [2.24] 1.22∗ [0.68] 1.75 [0.16] 1.71 [0.21]
RY Ori 4 460 1.99 [0.12] 1.43 [0.44] 0.460 [0.22] 0.993 [0.33] 1.01 [0.33]
UX Ori 5 517 10.8 [0.21] 6  ±  1 (2.73 [0.65]) (2.36 [0.30]) (1.08 [0.69])
V346 Ori 3 586 3.2  ±  0.4 ... ... (1.55 [0.42]) (1.18 [0.43])
V350 Ori 2 735 4.8  ±  0.2 5  ±  1 1.3  ±  0.2 2  ±  1 2.6  ±  0.2
XY Per 4 347 9.00 [0.28] 4.37∗ [0.87] 2.35 [0.41] 4.51 [0.19] 3.58 [0.14]
VV Ser 7 614 17.3 [0.06] 19.8 [0.18] 1.28 [0.25] 1.67 [0.20] 1.41 [0.26]
CQ Tau 5 1303 0.501 [0.19] 0.49  ±  0.08 0.10∗  ±  0.02 0.409 [0.18] 0.316 [0.11]
RR Tau 5 2103 169 [0.18] 253 [0.14] 24.4 [0.41] 42.4 [0.33] 37.7 [0.33]
RY Tau 5 1342 0.850 [0.09] 4.4  ±  0.3 (0.0694 [0.26]) (0.0993 [0.47]) (0.103 [0.50])
PX Vul 5 4201 2.76  ±  0.09 1.71 [0.28] 0.210 [0.62] 0.227 [0.27] 0.218 [0.22]
WW Vul 6 696 15.3 [0.07] 8.13 [0.22] 5.83 [0.29] 6.00 [0.42] 4.79 [0.50]
LkHa 234 4 12501 43.9  ±  0.6 36  ±  3 2.71 [0.19] 1.18 [0.62] 0.8  ±  0.2

Notes. Values from the data in Table A.2. Numbers in brackets are the line luminosity relative variabilities. Typical uncertainties are δ(σ/ ⟨ L ⟩ )  ~  0.06, 0.1, 0.2, and 0.1 for the Hα, [O i]6300, He i5876 and Na iD lines, respectively. Propagated uncertainties ( ± ; distance errors not considered) are indicated for the non-variable objects. Italic numbers refer to lines seen in absorption and values in parentheses are those lines shown both in absorption and emission. Only the values of the most frequent absorption/emission behaviour are considered in these cases to derive the mean values. “...” Indicates that the line is not detected. The distances are from Montesinos et al. (2009) by default, the remaining ones are taken from

(*)

Indicates that there is at least one spectrum not showing the line.

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