Table A.6
Detected lines of CH2CHCN g.s.
Transition | Predicted | S ij | E u | v LSR | Δ v | T MB |
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frequency (MHz) | (K) | km s-1 | km s-1 | (K) | (K km s-1) | |
|
|||||||
91,9–81,8 | 83 207.507 | 8.89 | 22.1 | 5.01 | 0.242 | ||
Wide comp. | 3.5 ± 0.4 | 14 ± 1 | 0.12 | 1.8 ± 0.2 | |||
Narrow comp. | 5.2 ± 0.3 | 0.8 ± 0.4 | 0.12 | 0.78 ± 0.11 | |||
90,9–80,8 | 84 946.003 | 9.00 | 20.4 | 4.41 | 0.242 | ||
4.4 ± 0.4 | 11 ± 1 | 0.23 | 2.7 ± 0.2 | ||||
92,8–82,7 | 85 302.649 | 8.56 | 29.1 | 5.21 | 0.242 | ||
5.2 ± 0.3 | 9.5 ± 0.7 | 0.22 | 2.26 ± 0.14 | ||||
. . . | . . . | . . . | . . . | . . . | |||
140,14–130,13 | 131 267.475 | 14.00 | 47.5 | 2.51 | 2.082 | ||
142,13–132,12 | 132 524.586 | 13.70 | 56.4 | 14 | ... | ||
145,10–135,9 | 132 900.001 | 12.20 | 101.9 | 5.71 | 1.182 | ||
145,9–135,8 | 132 900.012† | 12.20 | 101.9 | 5.81 | ” | ||
6.1 ± 0.5 | 7.8 ± 0.9 | 1.02 | 8.4 ± 0.9 | ||||
146,9–136,8 | 132 905.283 | 11.40 | 125.6 | 5.11 | 1.022 | ||
146,8–136,7 | 132 905.283† | 11.40 | 125.6 | 5.11 | ′′ | ||
. . . | . . . | . . . | . . . | . . . | |||
212,20–202,19 | 198 258.130 | 20.80 | 113.6 | 2.71,12 | 6.302 | ||
216,16–206,15 | 199 396.979 | 19.30 | 183.0 | 4.71 | 2.252 | ||
216,15–206,14 | 199 396.985† | 19.30 | 183.0 | 4.71 | ′′ | ||
217,15–207,14 | 199 401.677 | 18.70 | 211.0 | 5.11 | 2.452 | ||
217,14–207,13 | 199 401.677† | 18.70 | 211.0 | 5.11 | ′′ | ||
. . . | . . . | . . . | . . . | . . . |
Notes. Emission lines of CH2CHCN ground state present in the spectral scan of the Orion-KL from the radio-telescope of IRAM-30 m. 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 the line width, Col. 7 main beam temperature, and Col. 8 shows the area of the line. 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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