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Table 6

Selected CO, water and H2 lines with their observed fluxes (Salyk et al. 2007; Najita et al. 2010; Zhang et al. 2013) in the near- and mid-IR wavelength range from the “standard model” (model 1) and the model with 100 times higher gas mass inside 4 AU (model 14).

Species λ Line Obs. Model line flux
[μm] ident. F line [10-18 W/m2]
model 1 model 14

CO 4.700 v = 1−0 P4 7.2 3.33(−1) 50.8
CO 4.759 v = 2−1 P4 n.a. 7.66(−2) 25.1
CO 5.041 v = 1−0 P36 n.a. 2.80(−2) 35.7
o-H2 17.036 S(1) 12.1 3.43(−1) 4.71
o-H2O 17.36 1129−10110 n.a. 3.21(−1) 6.91
o-H2O 23.86 982−871 466.91 2.19 20.1
o-H2O 30.87 854−743 188.31 5.00 23.7

Notes. n.a. denotes not available.

(1)

At the low resolution of Spitzer, the observed fluxes are for a blend of multiple water lines, while the model flux is for the individual line.

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