Table A.7
Optical depth in the V -band for the ten best MM1 pre-burst models along the mid-plane and along the line of sight toward the center.
| Model | inc [°] |  |
 |
 |
|---|---|---|---|---|
| eGYXcOh8_02 | 19.3 | 360 | 3200 | 380 |
| 90Yt0exl_03 | 24.1 | 1.2 × 106 | 1.2 × 106 | 390 |
| PUyhjE8Z_02 | 11.3 | 30 | 11 000 | 360 |
| nTRTrE7X_02 | 18.1 | 1700 | 9300 | 420 |
| nTRTrE7X_03 | 23.3 | 1700 | 9300 | 510 |
| TJyUR9bA_02 | 14.5 | 2 | 11 000 | 240 |
| 4kW1TtMH_04 | 30.6 | 3.4 × 105 | 3.5 × 105 | 830 |
| lQ0YS3aF_02 | 13.5 | 1.2 × 105 | 1.4 × 106 | 889 |
| qWHuujku_05 | 46.8 | 6.2 × 105 | 6.6 × 105 | 920 |
| qWHuujku_06 | 50.0 | 6.2 × 105 | 6.6 × 105 | 1200 |
| Mean model | 21.8 | 3300 | 11 000 | 430 |
Notes. The intrinsic extinction dominates the total extinction (including the interstellar extinction) by far, as indicated by the huge values in the V -band. For τmid-plane the contribution of the disk is given separately. For some models, τdisk almost covers the total extinction (along the line of sight), whereas for some models the contribution of the envelope (which is the same as 
) is the dominant one. We note that the optical depths are given for the pre-burst, during the burst the optical depths may be slightly lower because of dust sublimation.
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