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Table 1.

Best-fit projected rotational velocities as derived from the disentangled spectra of HD 152219 and comparison with previous determinations.

Line v sin irot (km s−1)
Primary Secondary
Si IVλ 4089 163
Si IVλ 4212 135
O IIλ 4254 166 104
C IIλ 4267 166 80
O IIIλ 4277 169
N IIIλ 4379 156
O IIλ 4610 148
N IIIλ 4641 161
O IIIλ 5592 165
He Iλ 3820 184 104
He Iλ 4026 170
He Iλ 4143 172
He Iλ 4387 172
He Iλ 4471 168
He Iλ 4713 177
He Iλ 4922 167
He Iλ 5016 170 88
He Iλ 5875 170 97
He Iλ 6678 170
He Iλ 7065 166 98

Mean (metal lines) 159 ± 11 92 ± 17
Mean (He I lines) 171 ± 5 97 ± 7
Mean (all lines) 166 ± 10 95 ± 9

Conti & Ebbets (1977) 250
Levato & Morrell (1983) 160
Sana et al. (2006)
 He I lines 190 ± 10
 Si IVλ 4089 150 ± 10
 O IIIλ 5592 175 ± 10
 He IIλ 4542 130 ± 10
 He IIλ 4686 160 ± 10

Notes. The values quoted by Conti & Ebbets (1977) were obtained by visual comparison with standards and the values quoted by Levato & Morrell (1983) were obtained by visual comparison with the standards given by Slettebak et al. (1975). The values of Sana et al. (2006) were estimated through a comparison of the measured Full Widths at Half Maximum (FWHMs) of the various lines with those measured, for a range of v sin irot, on model spectra of equivalent effective temperature and gravity computed using the codes TLUSTY and SYNSPEC.

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