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Table C.1

Optical depths and abundance ratios for SO, 13CO, OCS, and CH3CN lines with respect to their rare isotopologue lines in each substructure of NGC 7538S and IRS1-mmS

Species α MM1 MM2 MM3 JetN JetS IRS1−mmS
(172 ± 23 K) (137 ± 14 K) (50 K) (150 K) (150 K) (162 ± 14 K)

τ SO (65 → 54) 44.5 7.5 24 6.5 10
N SOτ / N 33SO 127 112.20± 0.96 94.46± 10.42 638.08 409.18 132.30± 21.26
N SO / N 33SO 2.52± 0.02 12.59± 1.39 26.59 62.86 13.23± 2.13

13.5 9 9 8 8
N 13COτ / N C18O 8.3 16.07± 0.52 17.58± 0.02 12.54 13.84± 0.52 16.00± 0.95
N 13CO / N C18O 1.19± 0.04 1.95± 0.00 1.39 1.73± 0.06 2.00± 0.12

τ OCS (18 → 17) 4.5 5.5 36 38 15 4
N OCSτ / N O13CS 73.5 76.71± 1.88 72.81± 16.34 69.24± 1.17 159.60 72.06 86.40± 27.69
N OCS / N O13CS 16.86± 0.41 13.18± 2.96 1.92± 0.03 4.20 4.80 21.20± 6.80

τ CH3CN (122 → 112) 16 3 29 7
73.5 70.22± 7.06 78.13± 2.02 119.60 71.88± 5.30
4.39± 0.44 24.75± 0.64 4.12 10.26± 0.76

Notes.1)

(†)

or

(⋆)

mark the estimations with or without optical depth correction, respectively. 2) () come from the 3σ limit of the non-detection or partly absorption of C18O in IRS1-mmS. 3) The ratios α between isotopes of 12C /13C and 16O /18O are provided from the Galactic ISM ratio measured in Giannetti et al. (2014) (with RGC(NGC 7538) ~ 9.7 kpc), while 32S /33S is provided from the solar system ratio measured in Lodders (2003). 4) Uncertainties on the measured values are typically 10% as determined from Trot, partition function Q(Trot), and Gaussian fit to TB(υ)dυ.

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