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Table 1
Disk models used to compute emergent Stokes spectra.
| Model | τ r | τ z | Illumination |
|
|
|||
| A | 103 | 10 | Self-emitting |
| B | 104 | 102 | Self-emitting |
| Ai | 103 | 10 | Self-emitting + star illumination |
| Bi | 104 | 102 | Self-emitting + star illumination |
Notes. All models are isothermal, with opacity equal to unity, and ϵ = 10-4.
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