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Table 1

Molecular inventory of W Aql from HIFI observations.

Molecule Transition Frequency E up η mb I mb θ I model / I mb
[GHz]     [K] [K km s-1] [′′]

CO 6 → 5 691.473 116 0.75 14.1 30.7 1.03
10 → 9 1151.985 304 0.64 14.7 18.4 1.10
16 → 15 1841.345 752 0.70 15.9 11.5 1.01
13CO 6 → 5 661.067 111 0.75 1.3 32.1 0.87
10 → 9 1101.349 291 0.74 0.95 19.3 1.03
o-H2O 11,0 → 10,1 556.936 61 0.75 2.0 38.1 0.68
31,2 → 30,3 1097.365 250 0.74 2.2 19.3 1.50
31,2 → 22,1 1153.127 250 0.64 3.7 18.4 1.40
32,1 → 31,2 1162.911 306 0.64 1.8 18.2 0.68
p-H2O 11,1 → 00,0 1113.343 53 0.64 4.4 19.1 0.87
HCN 13 → 12 1151.452 387 0.64 3.5 18.4 1.03
H13CN 8 → 7 690.551 149 0.75 0.63 30.7 1.00
SiO 16 → 15 694.294 284 0.75 1.1 30.6 1.07
29SiO 13 → 12 557.179 187 0.75 0.25 38.1 1.00
o-NH3 10 → 00 572.498 27 0.75 0.85 37.1 1.06

Notes. Eup is the excitation energy of the upper transition level, ηmb is the main beam efficiency (see Eq. (1)), Imb is the integrated intensity (uncertainties are taken to be 20%), θ is the full-width half-power beam width, and Imodel/Imb is the ratio of modelled to observed integrated intensities.

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