Table 7
Stellar diameters estimated from the 25% iso-intensity levels of Fig. 13–15.
| Spectral | φ25% (mas) | φ25% (mas) | Δ(φ25%) /φ25% |
| band | Φ = 0.0 | Φ = 0.2 | |
| number | (epoch A) | (epoch B) | |
|
|
|||
| 1 | 5.01 ± 0.15 | 5.67 ± 0.19 | 0.13 ± 0.04 |
| 2 | 4.95 ± 0.16 | 5.64 ± 0.17 | 0.14 ± 0.03 |
| 3 | 4.76 ± 0.21 | 5.57 ± 0.23 | 0.17 ± 0.05 |
| 4 | 4.73 ± 0.20 | 5.57 ± 0.23 | 0.18 ± 0.05 |
| 5 | 4.84 ± 0.21 | 5.57 ± 0.23 | 0.15 ± 0.05 |
| 6 | 4.90 ± 0.18 | 5.57 ± 0.23 | 0.14 ± 0.04 |
Notes. Diameter values were averaged over the PAs. Results are expressed as μ ± 1σ, where μ is the average and σ is the standard deviation computed over all the PAs. The fourth column represents the relative variation of stellar diameter between epochs A and B, relatively to epoch A.
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