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Table 6

Total line fluxes [W m−2], column densities 〈Ncol〉 [cm−2], emission temperatures 〈Tg〉 [K], and emitting radii 〈r1 − r2〉 [au] of selected molecules, affected by stellar UV luminosity, X-ray luminosity, and mass-accretion rate, considering all lines between 13 and 17.7 µm.

Fiducial model High(1) LUV High(1·3) LX High(1) acc Old ProDiMo(2)
6.9(18) 1.9(−17) 6.9(−18) 6.9(−18) 3.6(−18)
OH 〈log10 Ncol 16.8 16.8 16.8 16.8 16.8
〈Tg 1700 1760 1700 1710 1460
r1r2 0.12–0.55 0.15–1.13 0.12–0.56 0.14–0.57 0.10–0.54

1.1(16) 1.5(−16) 1.1(−16) 1.5(−16) 1.2(−16)
H2O 〈log10 Ncol 19.1 19.0 19.0 19.1 19.0
〈Tg 620 640 620 650 600
r1 − r2 0.11–0.37 0.12–0.43 0.11–0.38 0.11–0.36 0.11–0.31

2.5(17) 2.1(−17) 3.0(−17) 2.6(−17) 9.3(−17)
CO2 〈log10 Acol 18.0 17.9 18.0 18.0 18.1
〈Tg 270 270 270 270 310
r1 − r2 0.39–0.87 0.38–0.89 0.36–0.86 0.40–0.87 0.26–0.65

8.5(17) 4.7(−17) 8.1(−17) 2.5(−16) 1.0(−18)
HCN 〈log10 Acol 17.5 17.1 17.5 18.1 14.9
〈Tg 580 570 550 660 590
r1 − r2 0.10–0.19 0.10–0.21 0.10–0.20 0.09–0.18 0.11–0.31

5.7(17) 3.1(−17) 1.0(−16) 1.5(−16) 1.3(−18)
C2H2 〈log10 Acol 16.9 16.3 17.2 17.2 13.8
〈Tg 740 740 690 770 410
r1 − r2 0.08–0.13 0.08–0.72 0.08–0.12 0.08–0.13 1.1–6.2

Notes. Increased by a factor of three with respect to the parameter value given in Table 4.(2): Same model parameters as the fiducial model, but before the code changes as described in Sect. 2.(3): A higher value of the parameter acc does not change LUV in the model, whereas in nature it should.

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