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

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Table D.1

Collected line luminosities from the literature.

Target	[OI] 0.63 µm [10⁻⁵ L_⊙]	o–H₂ 2.12µm [10⁻⁵ L_⊙]	distance [pc]
TW Hya	0.933 ± 0.187¹	0.011 ± 0.001^2,3	59.8
LkCa 15	0.871 ± 0.174¹	0.131 ± 0.015²	156.9
GM Aur	1.700 ± 0.170⁴	0.039 ± 0.001⁵	159.0
AA Tau	0.468 ± 0.047⁴	0.196 ± 0.006⁵	140.0
V773 Tau	13.804 ± 1.380⁴	0.139 ± 0.005⁵	131.0
CS Cha	2.240 ± 1.200⁶	0.168 ± 0.008⁷	160.0

Notes. References:⁽¹⁾ Fang et al. (2018).⁽²⁾ Bary et al. (2003);⁽³⁾ Nomura & Millar (2005);⁽⁴⁾ Simon et al. (2016);⁽⁵⁾ Beck & Bary (2019);⁽⁶⁾ Manara et al. (2014);⁽⁷⁾ Bary et al. (2008)

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