Interpreting molecular hydrogen and atomic oxygen line emission of T Tauri disks with photoevaporative disk-wind models

Open Access

Table 1

Model names and parameters.

Model name	L_acc (L_⊙)	Wind g/d ratio^(a)
PE-1	2.6 × 10⁻²	100
PE-2	0.31	100
PE-3	1.0	100
PE-1 gd	2.6 × 10⁻²	1000
PE-2 gd	0.31	1000
PE-3 gd	1.0	1000

Notes. ^(a)Gas-to-dust mass ratio in the wind region.

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