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Table 1

CTTSs used for this study, listed following the order of the Herbig-Bell catalog of Orion population stars (HBC).

HBC Object i rot Ref. i disk Ref. Vbe[O I] Vb[N II] Ref. FWHM(Hα) FWQM(He I) BAc(Hα) BAe(He I)
deg deg km s-1 km s-1 km s-1 km s-1 km s-1 km s-1

25 CW Tau –147 –109 12 465 290 –110 w
26 FP Tau –86 10 233 122 –47 –84
28 CY Tau 72 1 31 18 –138 10 189 91 w –161
30 DD Tau –79 –80 10 195 69 –50 –58
32 BP Tau 32 2 36 18 –31 10 315 70 w w
33 DE Tau 57 2 –148 10 300 125 –55 w
34 RY Tau 66 19 –115 12 450 w –40
35 T Tau N 15 1 20 6 –180 15 275 225 –190
36 DF Tau 50 2 –103 –84 12 295 75 –63 –163
37 DG Tau 58 2 32 18 –276 –219 10 225 285 –200 –383
38 DH Tau 58 1 –50 12 167 w
43 UX Tau A 60 1 46 23 125 w –155 –95
45 DK Tau 44 2 –138 10 320 65 –45 –209
48 HK Tau B 85 16 –22 –17 13 37 51 w
HH 30* 82 18 –19 –12 13 50 57 w
49 HL Tau 40 24 –198 –171 13 239 275 –148 –300
50 XZ Tau –133 –75 12 110 w –177
52 UZ Tau E 56 25 –155 –91 12 194 109 –44 –110
54 GG Tau 56 2 –138 10 240 190 –100 w
56 GI Tau 54 1 –69 10 165 68 –45 w
57 GK Tau 46 2 –35 10 300 45 –30 –77
58 DL Tau 78 2 40 18 –203 –188 10 260 281 –150 –191
60 HN Tau –133 –81 12 289 150 w w
61 CI Tau 46 25 –179 10 228 202 –113 –167
63 AA Tau 69 2 75 26 –55 –41 10 210 75 –20 –70
65 DN Tau 30 2 –48 10 195 45 –58 w
67 DO Tau –121 10 200 58 –100 –158
418 HV Tau C 84 17 –41 –25 13 98 109 w
72 DQ Tau –52 10 240 115 w w
74 DR Tau 15 4 20 7 –186 –166 10 175 145 –225 –330
75 DS Tau –72 10 300 50 –40 –140
76 UY Aur –103 10 200 68 w –135
77 GM Aur 90 1 52 18 –19 10 315 140 –75
80 RW Aur A 37 2 –221 10 490 125 –75
85 GW Ori 30 5 10 7 180 w –379
250 GQ Lup 27 3 –38 22 297 67 –13
251 RU Lup 28 7 –171 –173 11 258 220 w
KH15D 84 14 –35 14 121 –7
568 TW Hya 18 9 8 8 –12 20 190 129 –45 –260
578 VZ Cha –16 21 166 74 w
590 HM 32 –14 11 173 58 w
254 AS 205 A 47 25 –237 11 183 269 –180
286 S CrA N <45 7 –139 11 426 120 –85
291 VV CrA –257 –175 11 218 226 –310
292 AS 353 A 20 27 –352 10 275 335 –250 –279

Notes. The first column gives the HBC object number. The following columns give the most common object name, the inclination derived from the stellar rotation (irot) and the corresponding reference, the inclination derived from the disk aspect angle (idisk) and the corresponding reference, the radial velocity of the blue edge (measured at 25% intensity) of the 630 nm [O I] line, the velocity of the blue peak of the [N II] 658.3 nm line, the reference to the forbidden-line data, the Hα FWHM line width, the FWQM width of the 587.6 nm He I line, the central velocity of the blueshifted wind absorption feature in the Hα emission line (BAc(Hα)), and the blue edge (measured at 25% depth) of the blueshifted wind absorption feature of the 1083 nm He I line (BAe(HeI)). w indicates that the corresponding feature could not be detected or measured.

Reference. (1) Bouvier et al. (1995); (2) Bouvier (2004, priv. comm.); (3) Broeg et al. (2007); (4) Alencar et al. (2001); (5) Shevchenko et al. (1998); (6) Ratzka et al. (2009); (7) Schegerer et al. (2009); (8) Akeson et al. (2011); (9) Alencar & Batalha (2002); (10) Hartigan et al. (1995); (11) Hamann (1994); (12) Hirth et al. (1997); (13) Appenzeller et al. (2005); (14) Hamilton et al. (2003); (15) Böhm & Solf (1994); (16) Stapelfeldt et al. (1998); (17) Stapelfeldt et al. (2003); (18) Guilloteau et al. (2011); (19) Isella et al. (2010); (20) Herczeg et al. (2007); (21) Krautter et al. (1990); (22) Appenzeller & Wagner (1989); (23) Tanii et al. (2012); (24) Kwon et al. (2011); (25) Andrews & Williams (2007); (26) Cox et al. (2013); (27) Curiel et al. (1997).

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