Table 4
Angular diameters obtained with VEGA/CHARA and the corresponding surface brightness.
| Star | (V − K)0 | θUD [mas] | χ 2 | U R | θLD [mas] | Sv[mag] |
|
|
||||||
| λ Aql | −0.265 ± 0.055 | 0.529 ± 0.003 | 1.0 | 0.301 | 0.544 ± 0.003 | 2.079 ± 0.030 |
| γ Lyr | −0.102 ± 0.072 | 0.742 ± 0.010 | 2.9 | 0.402 | 0.766 ± 0.010 | 2.544 ± 0.059 |
| γ Ori | −0.703 ± 0.097 | 0.701 ± 0.005 | 0.4 | 0.269 | 0.715 ± 0.005 | 0.909 ± 0.081 |
| 8 Cyg | −0.492 ± 0.147 | 0.229 ± 0.011 | 1.3 | 0.299 | 0.234 ± 0.011 | 1.456 ± 0.177 |
| ι Her | −0.459 ± 0.076 | 0.304 ± 0.010 | 1.2 | 0.280 | 0.310 ± 0.010 | 1.225 ± 0.082 |
| ζ Per | −0.592 ± 0.092 | 0.531 ± 0.007 | 1.2 | 0.343 | 0.542 ± 0.007 | 0.652 ± 0.081 |
| ζ Peg | −0.204 ± 0.055 | 0.539 ± 0.009 | 1.7 | 0.442 | 0.555 ± 0.009 | 2.076 ± 0.152 |
| δ Cyg | + 0.021 ± 0.055 | 0.766 ± 0.004 | 1.3 | 0.408 | 0.791 ± 0.004 | 2.318 ± 0.129 |
Notes. The systematical uncertainties for the two fast rotating stars, ζ Peg and δ Cyg, are of 0.039 mas and 0.047 mas, respectively (see Sect. 3.2).
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