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Table 6

Column densities, excitation temperatures, FWHM and vpeak derived at thepeak positions of CH3OH (position 2 inFig. 12).

Molecule Column density Tex FWHM vpeak Peak position (a)
(cm−2) (K) (km s−1) (km s−1)
COMs and O-bearing species

CH3OH (b) 1.0 (0.2) × 1019 120 (25) 4.5 9.0 2
13CH3OH 1.3(0.2) × 1017 120 (25) 4.5 9.0 1/2
CH3 18OH (c) <3.0 × 1016 100 4.5 9.0
CH2DOH (c) <4.0 × 1016 100 4.5 9.0
C2H5OH 6.7(2.0) × 1016 130 (60) 5.0 9.5 1
CH3OCHO 1.4(0.2) × 1017 110 (20) 4.5 9.0 1
CH3OCH3 2.4(0.2) × 1017 110 (20) 5.0 9.0 1
H2CO (b) 5.9(1.5) × 1017 160 (40) 8.0 9.0 1
H2 13CO 7.6(2.0) × 1015 160 (40) 8.0 9.0 1
t-HCOOH 4.0(0.5) × 1016 190 (50) 7.0 11.0 3
c-HCOOH (c) <3.3 × 1015 190 7.0 11.0 -
HDO (d) 6.8(2.0) × 1016 120 (25) 4.0 10.5

S-bearing species

H2CS 3.3(0.5) × 1016 140 (50) 5.5 9.0 1
33SO (e) 5.4(2.0) × 1015 130 (40) 6.5 10.0 3
SO2 (b) 7.3(0.2) × 1017 130 (40) 6.0 10.0 3
33SO2 (c) <8.1 × 1015 130 (40) 6.0 10.0
34SO2 3.3(1.0) × 1016 130 (40) 6.0 10.0 3
OCS (a) 2.4(0.4) × 1017 170 (50) 5.0 10.0 2
OC34S 1.1(0.2) × 1016 170 (50) 5.0 10.0 1

N-bearing species

HNCO 5.0(1.0) × 1016 150 (20) 6.5 10.5 3
HC3N 4.0(1.0) × 1015 210 (40) 7.0 10.0 3
CH3CN, v8=1 (f) 5.5(2.0) × 1016 140 (10) 7.0 10.5 2/3
13CH3CN (c) < 9.1 × 1014 140 7.0 10.5

Notes. Values are derived from synthetic spectrum fitting with CASSIS, with the assumption of LTE. (a)Positions of peak molecular emission are as represented in Fig. 12. (b)Column densities for optically thick lines derived using ISM ratios from Wilson & Rood (1994). (c)Upper limits were determined by setting Tex, FWHM, and vpeak, equal to that of a detected isotopologue. (d)To estimate a column density for HDO, the excitation temperature of methanol was assumed. (e)Both SO and 34SO had optically thick lines, so only the column density of 33SO could be derived, using Tex of 34SO2. (f)CH3CN, v8 =1, was used for the model fit of CH3CN because it is optically thick, and 13CH3CN was not detected.

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