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Table 1
Overview of the observed transitions.
Molecule | Trans. | E u | A ul | Freq. |
Ju–Jl | [K] | [s-1] | [GHz] | |
|
||||
CO | 2–1 | 16.6 | 6.910 × 10-7 | 230.538000 |
3–2 | 33.19 | 2.497 × 10-6 | 345.795989 | |
4–3 | 55.3 | 6.126 × 10-6 | 461.040768 | |
6–5 | 116.2 | 2.137 × 10-5 | 691.473076 | |
7–6 | 154.9 | 3.422 × 10-5 | 806.651806 | |
10–9 | 304.2 | 1.006 × 10-4 | 1151.985452 | |
13CO | 2–1 | 15.9 | 6.038 × 10-7 | 220.398684 |
3–2 | 31.7 | 2.181 × 10-6 | 330.587965 | |
4–3 | 52.9 | 5.353 × 10-6 | 440.765174 | |
6–5 | 111.1 | 1.868 × 10-5 | 661.067277 | |
8–7 | 190.4 | 4.487 × 10-5 | 881.272808 | |
10–9 | 290.8 | 8.797 × 10-5 | 1101.349597 | |
C18O | 2–1 | 15.8 | 6.011 × 10-7 | 219.560354 |
3–2 | 31.6 | 2.172 × 10-6 | 329.330553 | |
5–4 | 79.0 | 1.062 × 10-5 | 548.831010 | |
6–5 | 110.6 | 1.860 × 10-5 | 658.553278 | |
9–8 | 237.0 | 6.380 × 10-5 | 987.560382 | |
10–9 | 289.7 | 8.762 × 10-5 | 1097.162875 |
Notes.The level energies, Einstein A coefficients, and line frequencies are from the LAMDA, JPL and CDMS databases (Schöier et al. 2005; Pickett et al. 2010; Müller et al. 2005).
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