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Table 3.

Emission line radial velocity, FWHM, and equivalent width measurements.

July August Average
ID RV FWHM RV FWHM RVem −EW Vabs Vedge
He I 3704.00? −15. 332. −56. 307. 135 1.1 −210 −250
H I 3750.20 −129. 328. 16 0.6 −172 −283:
H I 3770.60 −102. 358. −85. 374. 75 1.8 −258 −400:
H I 3797.90 −105. 308. −10 0.4 −221 −310
He I 3819.60* −178. 361. −136. 228. 17 1.2 −252 −530
H I 3835.40* −147. 320. −104. 461. 32 1.2 −201 −370:
He I 3888.65 −149 457 −183 485: 20 10.4 −350 −660
H I 3970.10* −124. 325. −149. 310. 18 2.2 −193
He I 4026.20* −149. 342. −152. 342. 10 2.4 −248 −550
N IV 4057.76 −223. 273. −164. 148. −10 0.5
Si IV 4088.70* −182. 213. −173. 198. 2 1.7
N III 4097.30 −200. 154. −190. −4 2.0: −230 −438
H I 4101.74 −67. 373. −51. 285. 121: 5.2
Si IV 4116.10* −228. 364. −211. 233. −32 2.8
N III 4195.76 −234. 141. −266. 164. −66: 0.2
N III 4200.10 −162. 206. −165. 142. 13 0.6 −159: −260:
H I 4340.50* −149. 380. −119. 366. 42 7.9
N III 4379.20* −186. 260. −164. 226. −7 1.0
He I 4387.90* −198. 301. −135. 246. 13 1.6
He I 4471.50* −149. 389. −127. 362. 28 4.9 −275 −630
N III 4534.60* −194. 178. −149. 165. −22 0.4: −233: −280:
He II 4541.60 −145. 145. 29: 2.0: −182 −300:
N III 4634.14 −183 256 −188 252 −9 5.5
N III 4640.64 −197. 252. −195. 258. −16 9.4
He II 4685.6* −176. 333. −174. 326. 7 17.4
He I 4713.1* −146. 197. −130. 407. 28 1.6: −291 −500:
H I 4861.3* −171. 395. −167. 401. 11 18.2
He I 4921.9* −185. 335. −174. 371. 4 4.3
He I 5015.7* −162. 275. −149. 287. 15 1.7 −200:
He I 5047.7* −174. 184. −143. 237. 41 0.6
He II 5411.52 −150. 260. −169. 294. 15 1.9 −217 −433
He I 5875.66* −175. 444. −171. 464. 5 24.5 −304 −655
H I 6562.80 −184. 301. −176. 269. −1
H I 6562.80* −181. 466. −172. 461. 8 68.0
He I 6678.15* −176. 417. −185. 395. −6 18.0
He I 7065.20* −152. 467. −157. 450. 13 18.1 −306 −560
N IV 7109.35 −169. 181. 8 0.2:
N IV 7122.98 −160. 231. 0.3

Notes. Column 1: primary atomic identification and corresponding laboratory wavelength in Å; Cols. 2 and 4: RVs for the July and the August observations respectively, after applying the heliocentric corrections of +27 km s−1 for July and +24 km s−1 for of August; Cols. 3 and 5: corresponding full-widths at half maximum intensity. Columns 6–9: measurements performed on the combined July+August spectrum after correcting for the adopted −179 km s−1 systemic velocity of M 33. Column 6: RV of the emission lines; Col. 7: corresponding equivalent width; Col. 8: centroid of the P Cyg absorption component when present; and Col. 9: velocity of the P Cyg absorption edge (i.e. the location where the absorption reaches the continuum). RVs and FWHM’s are in units of km s−1; EWs are in units of Å, and the negative sign in the column heading indicates emission. Asterisk indicates the line was used to determine the RV of the system.

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