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Table 4
Values for the grid parameters of the four best fit models to the CO molecular emission data.
| T ⋆ | ϵ 1 | ϵ 2 | R t | Ṁ g | ψ dens | nH2O,crit/nH2 | |
| (K) | (R⋆) | (M⊙ yr-1) | |||||
|
|
|||||||
| 1 | 3500 | 0.2 | 0.9 | 5 | 1.0 × 10-4 | 0.005 | 8.5 × 10-5 |
| 2 | 3000 | 0.2 | 0.9 | 5 | 5.0 × 10-5 | 0.01 | 1.7 × 10-4 |
| 3 | 2500 | 0.2 | 0.9 | 5 | 2.0 × 10-5 | 0.025 | 4.0 × 10-4 |
| 4 | 2000 | 0.01 | 1.0 | 5 | 2.0 × 10-5 | 0.025 | 4.0 × 10-4 |
Notes.Listed are the stellar effective temperature T⋆, the powers of the 2-step power law ϵ1 and ϵ2, the transition radius Rt, the gas-mass-loss rate Ṁg, the dust-to-gas-ratio ψdens, and the critical H2O abundance nH2O,crit/nH2.
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