Table 1
Radiative-equilibrium temperatures at slab center and slab surface (in parentheses).
| p[dyn cm-2] | 0.01 | 0.1 | 0.5 | Model |
|
|
||||
| D = 200 km | 9754 (9757) | 7994 (8179) | 7010 (7556) | HI losses only, Tr = f(λ) |
| D = 1000 km | 9702 (9712) | 7403 (8047) | 6616 (7550) | |
| D = 5000 km | 9481 (9567) | 6778 (8022) | 6340 (7550) | |
|
|
||||
| D = 1000 km | 6458 (6291) | 6846 (6630) | 6593 (6778) | HI losses only, Tr = 6500 K |
| 1.03 | 31.6 | 252 | ||
|
|
||||
| D = 1000 km | 7156 (7150) | 7418 (6146) | 6734 (6409) | HI losses only, Tr = 8000 K |
| 0.015 | 2.28 | 208 | ||
|
|
||||
| D = 200 km | 9532 (9530) | 6773 (7277) | 5015 (6032) | HI + CaII losses, Tr = f(λ) |
| D = 1000 km | 9471 (9479) | 5450 (7026) | 4630 (6012) | |
| D = 5000 km | 9195 (9302) | 4874 (6995) | 4421 (5983) | |
Notes. f(λ) is the wavelength-dependent radiation temperature of the incident Lyman-continuum radiation. For the second and third set of models, the numbers below temperatures indicate the optical thickness of the 1D slab at the head of the Lyman continuum. All models shown here were computed with PRD in hydrogen and CaII lines.
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