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Table 5:

Column densities - OCS.

Species
Extended ridge Compact ridge Plateau Hot core
  $N \times 10^{15}$ (cm-2) N $\times$ 1015 (cm-2) $N \times 10^{15}$ (cm-2) N $\times$ 1015 (cm-2)
OCS 2.0 $\pm$ 0.5 3.0 $\pm$ 0.8 7.5 $\pm$ 1.9 15 $\pm$ 4
OCS assuming 32S/34S = 20 2.0 $\pm$ 0.5 14 $\pm$ 4 10 $\pm$ 3 60 $\pm$ 15
OCS assuming 12C/13C = 45 2.7 $\pm$ 0.5 18 $\pm$ 4 13.5 $\pm$ 3 45 $\pm$ 9
OCS (average) 2.4 $\pm$ 0.5 16 $\pm$ 4 11.8 $\pm$ 3 53 $\pm$ 10
OC34S 0.15 $\pm$ 0.03 0.70 $\pm$ 0.18 0.50 $\pm$ 0.13 3.0 $\pm$ 0.8
OC33S 0.050 $\pm$ 0.025 0.090 $\pm$ 0.045 0.10 $\pm$ 0.05 0.30 $\pm$ 0.15
O13CS 0.060 $\pm$ 0.015 0.40 $\pm$ 0.10 0.30 $\pm$ 0.08 1.0 $\pm$ 0.3
18OCS 0.010 $\pm$ 0.005 0.070 $\pm$ 0.035 0.030 $\pm$ 0.015 0.10 $\pm$ 0.05
O13C34S $\la$0.010 $\la$0.050 $\la$0.050 $\la$0.070
17OCS $\la$0.005 $\la$0.020 $\la$0.010 $\la$0.020
OC36S $\la$0.005 $\la$0.030 $\la$0.020 $\la$0.030
OCS $\nu _2$ = 1 ... ... ... 1.5 $\pm$ 0.4
OCS $\nu _3$ = 1 ... ... ... 0.15 $\pm$ 0.07

Notes. Column densities for the different OCS isotopologues and OCS vibrationally excited derived from our model of the different Orion's components (see text, Sect. 5.1).


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