Table 1:

Beam-averaged molecular column densities.

Species
Transition Wavelength Eu Intensitya Column density
    (microns) (K) (10-6 erg s-1 cm-2 sr-1) (1015 cm-2)

C18O
$J=7\rightarrow 6$ 390.2 147.5 2.6[1.1] 7.7[24,3.8]b
C18O $J=8\rightarrow 7$ 341.5 189.6 3.3[1.1] 15[72,5.5]b
C18O $J=9\rightarrow 8$ 303.6 237.0 11[3.9] 96[720,25]b - 10[43,5.4]c
C17O $J=8\rightarrow 7$ 333.7 194.1 1.4[1.1] 6.6[33,2.3]b
CH+ $J=1 \rightarrow 0$ 359.0 40.1 6.7[1.1] 0.0065[0.0058,0.0088]c
ortho-H2O 1 $_{10} \rightarrow 1_{01}$ 538.3 61.0 2.6[1.1] $\le$30[60,15]b,d
para-H2O 2 $_{11} \rightarrow 2_{02}$ 398.6 136.9 2.0[1.1] $\le$45[150,17]b,d
HCO+ $J=8\rightarrow 7$ 420.3 154.1 $\le$0.7e $\le$0.35[1.1,0.16]b,e
H2S 212 $\rightarrow$ 101 407.3 55.1 1.4[1.1] 0.031[0.023,0.052]c

Notes. (a) Intensities with uncertainty in between brackets. (b) Beam-averaged column densities using RADEX with n=105 cm-3 and T = 85 K, with estimations for 50 and 150 K in between brackets. (c) Beam-averaged column densities in the high-density (LTE) limit for 85 K, with estimations for 50 and 150 K in between brackets. (d) Note that the density (or temperature) could be higher than assumed, which would decrease the column density, and the para-H2O 2 $_{11} \rightarrow 2_{02}$ line could be affected by IR pumping. (e) We used the HCO+ $J=8\rightarrow 7$ line because the HCO+ $J=7\rightarrow 6$ line is possibly blended with an HCl $J=1 \rightarrow 0$ line. Column densities from 12CO and 13CO lines are uncertain due to high optical depth and are not listed.


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