Table A.12
Detected lines of CH2CHCN ν10 = 1 ⇔ (ν11 = 1,ν15 = 1).
Transition | Predicted | S ij | E u | v LSR 1 | Observed | Observed | Model |
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frequency (MHz) | (K) | km s-1 | frequency (MHz) | TMB (K)2 | TMB (K) | |
|
|||||||
91,9,0–81,8,0 | 83 116.219 | 8.89 | 830.7 | 4.4 | 83 116.4 | 0.02 | 0.01 |
91,9,1–81,8,1 | 83 527.527 | 8.89 | 834.3 | 1.9 | 83 528.4 | 0.03 | 0.01 |
90,9,0–80,8,0 | 84 834.239 | 8.99 | 829.0 | 7.4 | 84 833.6 | 0.01 | 0.01 |
92,9,0–82,8,0 | 85 222.373 | 8.55 | 837.7 | 3 | ... | ... | ... |
. . . | . . . | . . . | . . . | . . . | |||
140,14,0–130,13,0 | 131 110.736 | 14.00 | 856.1 | 22 | ... | ... | ... |
142,13,0–132,12,0 | 132 389.964 | 13.70 | 864.9 | 3.0 | 132 390.8 | 0.04 | 0.04 |
145,10,0–135,9,0 | 132 761.289 | 12.20 | 910.1 | 5 | ... | ... | ... |
145,9,0–135,8,0 | 132 761.289† | 12.20 | 910.1 | 5 | ... | ... | ... |
146,9,0–136,8,0 | 132 767.225 | 11.40 | 933.6 | 5 | ... | ... | ... |
146,8,0–136,7,0 | 132 767.225† | 11.40 | 933.6 | 5 | ... | ... | ... |
. . . | . . . | . . . | . . . | . . . | |||
212,20,0–202,19,0 | 198 041.306 | 20.80 | 922.0 | 16 | ... | ... | ... |
212,20,1–202,19,1 | 199 062.857 | 20.80 | 926.1 | 6.0 | 199 062.2 | 0.08 | 0.10 |
216,16,0–206,15,0 | 199 190.101 | 19.30 | 991.0 | 7.55,16 | 199 188.4 | 0.15 | 0.15 |
216,15,0–206,14,0 | 199 190.107† | 19.30 | 991.0 | 7.55,16 | 199188.4 | ” | 0.15 |
217,14,0–207,13,0 | 199 196.532 | 18.70 | 1018.8 | 4.0 | 199 197.1 | 0.14 | 0.13 |
217,15,0–207,14,0 | 199 196.532† | 18.70 | 1018.8 | 4.0 | 199197.1 | ” | 0.13 |
. . . | . . . | . . . | . . . | . . . |
Notes. Emission lines of CH2CHCN ν10 = 1 ⇔ (ν11 = 1,ν15 = 1) present in the spectral scan of the Orion-KL from the radio-telescope of IRAM-30 m. The quantum number ν corresponds with the vibrational level and takes the value ν = 0 and ν = 1 whether the state is ν10 = 1 or (ν11 = 1,ν15 = 1), respectively. Column 1 indicates the line transition, Col. 2 gives the predicted frequency in the laboratory, Col. 3 the line strength, Col. 4 upper level energy, Col. 5 observed radial velocities relative to the local system rest (vLSR), Col. 6 observed centroid frequencies assuming a vLSR of 5 km s-1, Col. 7 observed main beam temperature, and Col. 8 mean beam temperature obtained with the model. The superscripts are as follows: (This table is available in its entirety at the CDS. A portion is shown here for guidance regarding its form and content.)
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