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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