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Table 4
Best-fit model parameters for each epoch of our S Ori observations.
| Epoch | Φvis | Model | Φmod | τ V | Rin/RPhot | p | ΘPhot |
| (Al2O3) | (Al2O3) | (Al2O3) | [mas] | ||||
|
|
|||||||
| A | 0.40 | M24n | 0.40 | 2.5 | 2.0 | 2.4 | 8.5 |
| B | 1.89 | M22 | 0.25 | 1.0 | 1.8 | 3.3 | 10.0 |
| C | 1.95 | M21n | 0.10 | 1.4 | 2.3 | 3.7 | 8.8 |
| D | 2.01 | M21n | 0.10 | 1.5 | 2.4 | 3.0 | 8.9 |
| E | 2.10 | M22 | 0.25 | 1.4 | 1.8 | 3.0 | 10.5 |
| F | 2.16 | M23n | 0.30 | 1.1 | 2.2 | 3.6 | 10.1 |
| G | 2.22 | M23n | 0.30 | 1.2 | 1.8 | 2.7 | 10.1 |
| H | 2.29 | M25n | 0.50 | 1.2 | 1.8 | 2.5 | 8.5 |
| I | 2.91 | M22 | 0.25 | 1.4 | 1.7 | 3.0 | 10.2 |
| J | 3.00 | M22 | 0.25 | 1.2 | 1.8 | 2.5 | 11.1 |
| K | 3.13 | M25n | 0.50 | 2.4 | 1.5 | 3.0 | 9.0 |
| L | 3.19 | M23n | 0.30 | 1.8 | 2.2 | 2.5 | 10.9 |
| M | 3.82 | M22 | 0.25 | 1.4 | 1.7 | 2.9 | 10.8 |
| N | 3.96 | M25n | 0.50 | 1.5 | 2.1 | 2.5 | 8.7 |
Notes. The table lists the star, the epoch, the phase at the epoch, the optical depth τV, the inner boundary radius Rin/RPhot, the density distribution p, and the continuum photospheric angular diameter ΘPhot.
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