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Table 3

Emission lines of SiS, 29SiS, and SiS v = 1 present in the frequency range of the Orion KL survey.

Molecule Observed TMB Trasition Rest Eu Sij
vLSR (km s-1) (K) (K km s-1) J Frequency (MHz) (K)

SiS 12.5 0.29 6.1  ±  0.3 5−4 90771.558 13.1 5.00
16.7 0.53 11.5  ±  0.5 6−5 108924.294 18.3 6.00
15.5 1.34 30  ±  1 8−7 145227.045 31.4 8.00
16.5 2.141 43  ±  1 9−8 163376.773 39.2 9.00
16.2 2.42 ... 11–10 199672.219 57.5 11.00
11.1 3.10 ... 12–11 217817.651 68.0 12.00
8.92 20.0 ... 13–12 235961.363 79.3 13.00
17.7 4.45 ... 14–13 254103.213 91.5 14.00
15.2 4.25 ... 15–14 272243.058 104.5 15.00
29SiS 16.6 0.019 ... 5−4 89103.781 12.8 5.00
3 ... ... 6−5 106923.019 18.0 6.00
16.1 0.087 ... 8−7 142558.873 30.8 8.00
4 ... ... 9−8 160375.213 38.5 9.00
5 ... ... 12–11 213816.228 66.7 12.00
13.1 0.25 ... 13–12 231626.772 77.8 13.00
6 ... ... 14–13 249435.521 89.8 14.00
12.9 0.24 ... 15–14 267242.338 102.6 15.00
SiS v=1 noise level ... ... 5−4 90329.891 13.0 5.00
2 ... ... 6−5 108394.292 18.2 6.00
12.4 0.12 ... 8−7 144520.370 31.2 8.00
13.3 0.467 ... 9−8 162581.760 39.0 9.00
11.9 0.17 ... 11–10 198700.526 57.2 11.00
8 ... ... 12–11 216757.615 67.6 12.00
14.8 0.31 ... 13–12 234812.983 78.9 13.00
13.8 0.36 ... 14–13 252866.487 91.0 14.00
1 ... ... 15–14 270917.984 104.0 15.00

Notes. Column 2 gives the observed (centroid) radial velocities; Col. 3: peak line temperature; Col. 4: integrated intensity; Col. 5: line transition; Col. 6: calculated rest frequencies; Col. 7: energy of the upper level; Col. 8: line strength.

(1)

Blended with CH3OCOH.

(2)

Blended with 13CH3OH.

(3)

Blended with U line.

(4)

Blended with (CH3)2CO.

(5)

Blended with 34SO2.

(6)

Blended with CH3OH.

(7)

Blended with 33SO2.

(8)

Blended with CH3CH2CN b type.

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