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Home All issues Volume 572 (December 2014) A&A, 572 (2014) A44 Full HTML
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Table A.14

Detected lines of vinyl isocyanide (CH2CHNC).

Transition Predicted S ij E u v LSR 1 Observed Observed Model
frequency (MHz) (K) km s-1 frequency (MHz) TMB (K)2 TMB (K)
92,8–82,7 92 222.557 8.56 31.0 2.74 92 223.3 0.02 0.01
93,7–83,6 92 376.457 8.00 42.2 8.823 92 375.3 0.03 0.01
96,4–86,3 92 379.404 5.00 102.0 5.487 92 379.3 0.01 0.01
96,3–86,2 92 379.404† 5.00 102.0 5.487 92 379.3 0.01 0.01
93,6–83,5 92 386.902 8.00 42.2 6.95 92 386.3 0.02 0.01
. . . . . . . . . . . . . . .
132,12–122,11 133 062.524 12.70 53.6 3.416 133 063.2 0.04 0.03
133,10–123,9 133 566.376 12.30 64.8 6.48 133 565.7 0.04 0.03
132,11–122,10 134 563.575 12.70 53.9 4.757 134 563.7 0.08 0.04
140,14–130,13 141 702.008 14.00 51.3 5.82 141 701.6 0.04 0.04
. . . . . . . . . . . . . . .
192,17–182,16 198 094.397 18.80 103.3 4.5010 198 094.8 0.09 0.10
191,18–181,17 198 245.681 18.90 97.7 8.79 198 242.9 0.10 0.10
203,18–193,17 205 532.002 19.50 123.5 8.41 205 529.7 0.10 0.10
211,21–201,20 208 561.673 20.90 112.7 2.99 208 563.0 0.15 0.12
. . . . . . . . . . . . . . .

Notes. Emission lines of vinyl isocyanide (CH2CHNC) 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 relatives (vLSR), Col. 6 observed centroid frequencies assuming a vLSR of 5 km s-1, Col. 7 observed mean 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.)

(†)

Blended with the last one.

(1)

Peak line observed velocity.

(2)

Peak line intensity.

(3)

Blended with HCOOCH3 νt = 1.

(4)

Blended with HCOOCH3.

(5)

Blended with H13COOCH3.

(6)

Blended with CH2CHCN.

(7)

Blended with U-line.

(8)

Blended with SO18O.

(9)

Blended with DCOOCH3.

(10)

Blended with O-H2CS.

(11)

Blended with HCDCHCN.

(12)

Blended with CH3CH2CN.

(13)

Blended with (CH3)2CO.

(14)

Blended with CH3CH2C15N.

(15)

Blended with HCOO13CH3.

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