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Table 1

Properties of the observed lines.

λ (μm) Transition ncrit (cm−3) Eu/k (K) Aij (s−1)
CO 649.7 J = 4− 3 8 (04) 55.3 6.13 (–06)
CO 520.2 J = 5− 4 2 (05) 83.0 1.22 (–05)
CO 433.6 J = 6− 5 3 (05) 116 2.14 (–05)
CO 371.7 J = 7− 6 4 (05) 155 3.42 (–05)
CO 325.2 J = 8− 7 6 (05) 199 5.13 (–05)
CO 289.1 J = 9− 8 8 (05) 249 7.33 (–05)
CO 260.2 J = 10− 9 1 (06) 304 1.01 (–04)
CO 236.6 J = 11− 10 1 (06) 365 1.34 (–04)
CO 216.9 J = 12− 11 2 (06) 431 1.74 (–04)
CO 200.3 J = 13− 12 2 (06) 503 2.20 (–04)
CO 137.3 J = 19 18 5 (06) 1050 5.70 (–04)
13CO 546.2 J = 5− 4 1 (05) 79.3 1.07 (–05)
13CO 455.2 J = 6− 5 2 (05) 111 1.87 (–05)
13CO 390.2 J = 7− 6 4 (05) 148 2.99 (–05)
13CO 341.5 J = 8− 7 5 (05) 190 4.49 (–05)
13CO 303.6 J = 9− 8 7 (05) 238 6.41 (–05)
13CO 273.2 J = 10− 9 1 (06) 291 8.80 (–05)
13CO 248.4 J = 11− 10 1 (06) 349 1.17 (–04)
13CO 226.9 J = 12− 11 2 (06) 412 1.52 (–04)
13CO 209.5 J = 13− 12 2 (06) 481 1.92 (–04)

Notes. The table lists: wavelength (λ), transition, critical density (ncrit), upper level energy (Euk), and Einstein coefficient (Aij). Numbers in parentheses are power of 10. The critical densities have been calculated with ortho-H2 (Yang et al. 2010) and with a temperature of 100 K. The rest frequencies for CO were determined by Winnewisser et al. (1997) and for 13CO by Cazzoli et al. (2004).

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