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Table 6

Visibility ratios dV2/ ⟨ V2 ⟩  calculated for different B sub-spectral types and luminosity classes, with several equator-to-polar radius ratios Re/Rp. The visibility ratios are calculated at λ = 5500  Å for two baselines and apparent visible magnitudes V.

B = 156 m B = 300 m

Re/Rp Re/Rp
D (pc) θo (mas) 1.05 1.10 1.25 1.05 1.10 1.25

B0V
316 0.203 0.036 0.070 0.143 0.151 0.274 0.550
501 0.128 0.015 0.029 0.055 0.056 0.102 0.210
B0III
457 0.195 0.036 0.063 0.131 0.135 0.252 0.510
724 0.123 0.015 0.026 0.052 0.050 0.094 0.194
B2V
174 0.262 0.063 0.117 0.242 0.277 0.504 0.954
275 0.165 0.024 0.044 0.093 0.096 0.176 0.362
B2III
302 0.250 0.056 0.107 0.218 0.248 0.453 0.868
479 0.158 0.021 0.041 0.084 0.085 0.161 0.327
B8V
57 0.433 0.036 0.067 0.139 0.145 0.269 0.536
91 0.273 0.015 0.028 0.054 0.055 0.099 0.204
B8III
115 0.414 0.173 0.315 0.627 1.329 1.750 1.966
182 0.261 0.062 0.116 0.240 0.274 0.499 0.946

Notes. D is the distance and θo is the angular diameter. For a given spectral type, the first line is for V = 4 mag and the second for V = 5 mag.

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