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Table 2

List of Be-type stars observed in the Magellanic Cloud clusters NGC 346, NGC 330, NGC 2004 and the N 11 region.

Star Spectral S/N vsini Note Star Spectral S/N vsini Note
Type (km s-1) Type (km s-1)

NGC 346-004 Be(B1:) 307 266 ... NGC 330-065 B1-3e 39 284 1
NGC 346-008 B1e 187 299 ... NGC 330-068 B1.5e 30 23 1
NGC 346-009* B0e 114 181 ... NGC 330-069 B3 IIIe 40 193 ...
NGC 346-023* B0.2:e 130 50 ... NGC 330-070 B0.5e 39 348 1
NGC 346-024 B2e:shell 160 190 ... NGC 330-076 B3e 35 62 1
NGC 346-036 B0.5 Ve 142 287 ... NGC 330-083 B3 IIIe 38 140 ...
NGC 346-041 B2e 130 144 1 NGC 330-085 B3:e 38 191 1
NGC 346-045 B0.5 Vne 135 181 ... NGC 330-087 Be (B0-3) 24 214 1
NGC 346-048 Be (B3 shell) 121 158 2 NGC 330-091 B0e 32 272 1
NGC 346-061 B1-2e 118 336 1 NGC 330-096 B1-3e 26 175 1
NGC 346-064 B1-2e 117 108 1 NGC 330-100 Be (B0-3) 25 373 1
NGC 346-065 B3e 105 222 1 NGC 330-112 B1-3e 24 262 1
NGC 346-067 B1-2e 105 351 1
NGC 346-068 B0 Ve 109 378 1 NGC 2004-023 B2e 169 102 ...
NGC 346-069 B1-2e 102 186 ... NGC 2004-025 B2e 153 83 ...
NGC 346-072 B1-2e 112 102 ... NGC 2004-027 B0e 148 182 ...
NGC 346-073 B1-2e 110 190 ... NGC 2004-035 B1:e 125 244 ...
NGC 346-076 B2e 106 237 1 NGC 2004-039 B1.5e 106 212 ...
NGC 346-089 B1-2e 91 79 ... NGC 2004-048* B2.5e 86 244 ...
NGC 346-091 B1e 77 49 ... NGC 2004-056 B1.5e 74 229 ...
NGC 346-095 B1-2e 97 227 1 NGC 2004-058 O9.5 Ve 125 195 ...
NGC 346-096 B1-2e 100 343 1 NGC 2004-067 B1.5e 56 237 ...
NGC 346-110 B1-2e 93 243 1 NGC 2004-083 B1.5:e 73 194 1
NGC 2004-089 B2.5e 67 288 ...
NGC 330-025* B1.5e 93 250 ... NGC 2004-092 B2e 61 171 ...
NGC 330-029 B0.2 Ve 85 209 ... NGC 2004-096 B1.5e 63 245 ...
NGC 330-031 B0.5 Ve 98 178 ... NGC 2004-115* B2e 111 15 3
NGC 330-034 B1-2e 54 231 1
NGC 330-044 B1-2e 25 184 1 N 11-073 B0.5e 143 222 ...
NGC 330-050 B3e 67 214 1 N 11-074* B0.5e 149 102 ...
NGC 330-054 B2e 44 147 1 N 11-078 B2e 153 93 2
NGC 330-060 B2.5e 37 88 1 N 11-081 B0:ne 135 363 1
NGC 330-062 B3e 43 241 1 N 11-090* B2e 119 118 ...
NGC 330-064 B3:e 23 269 1

Notes. Spectral types and projected rotational velocities (vsini) are taken from Hunter et al. (2008), unless stated otherwise.

(*)

Value of vsini has been redetermined (see Sect. 2.2).

(1)

Omitted: no reliable measurements of the Mg ii/Si iii or He ii spectrum.

(2)

Omitted: the presence of a strong shell spectra.

(3)

Omitted: not a classical Be-type star. Short period binary.

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