Table B.1
CO and SiO integrated intensity values, and H2 level populations measured over a beam of 24′′ centred on the SiO knot position.
| Observable | Species | Line | SiO knot |
|
|
|||
 (K km s-1) |
CO | (3–2) | 113.4 ± 17.0 |
| CO | (4–3) | 117.3 ± 17.6 | |
| CO | (6–5) | 115.2 ± 17.3 | |
| CO | (7–6) | 95.2 ± 14.3 | |
| CO | (11–10) | 22.9 ± 3.4 | |
| CO | (16–15) | 3.4 ± 0.5 | |
| (K km s-1) |
SiO | (5–4) | 10.5 ± 1.1 |
| SiO | (6–5) | 5.6 ± 0.6 | |
| SiO | (8–7) | 2.5 ± 0.3 | |
|
|
|||
| Observable | Species | Level | SiO knot |
|
|
|||
| ln (N/g) | H2 | (0, 0) | 43.5 ± 1.2 |
| H2 | (0, 1) | 41.0 ± 1.3 | |
| H2 | (0, 2) | 40.3 ± 1.3 | |
| H2 | (0, 3) | 38.9 ± 1.4 | |
| H2 | (0, 4) | 38.2 ± 1.4 | |
| H2 | (0, 5) | 36.7 ± 1.4 | |
| H2 | (0, 6) | 35.7 ± 1.4 | |
| H2 | (0, 7) | 34.6 ± 1.5 | |
Notes. This means that the CO (16−15) (nominal resolution of 16.̋3) and SiO (nominal resolution of 28′′) data were a posteriori corrected assuming the emission is extended over the largest beam. As such, the initial data were multiplied by (16.3/24)2 and (28/24)2. The uncertainties are given. The integrated intensities were calculated between −4.5 and 50 km s-1. The CO and SiO integrated intensities correspond to a filling factor of 1.
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