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Table 1

CO line observation parameters and velocity-integrated line flux of the outflow components: jet, shock, outflow cavity.

CO ν E u Telescope HPBW F eff B eff Δν rms Jet Shock Outflow cavity
transition (GHz) (K) (”) () (TmbmK) K km s-1 K km s-1 K km s-1

1–0 115.2713 5.5 IRAM 21.4 0.95 0.78 0.51 11 1.38 17.0
2–1 230.5380 16.6 IRAM 20.0 0.92 0.45 1.30 50 6.14 67.8
3–2 345.7959 33.2 JCMT 20.0 1.0 0.67 0.54 77 9.38 101.8
4–3 461.0408 55.3 JCMT 10.7 1.0 0.45 0.61 509 23.31 252.8
5–4 576.2679 83.0 HIFI 37.4 0.96 0.75 0.14 7 5.21 3.4 33.9
9–8 1036.9124 248.9 HIFI 20.5 0.96 0.74 0.14 11 7.28 12.5 42.1
12–11 1381.9950 431.3 SOFIA 21.7 0.95 0.55 0.04 81 2.33 8.1 13.7
13–12 1496.9229 503.1 SOFIA 17.7 0.97 0.67 0.037 48 3.05 12.2 20.5
14–13 1611.7935 580.5 HIFI 13.2 0.95 0.71 0.19 55 3.32 10.5 18.2
16–15 1841.3455 751.7 SOFIA 14.5 0.97 0.65 0.030 58 2.83 13.9 21.0

13CO

2–1 220.3987 15.9 IRAM 11.2 0.92 0.61 2.7 8 5.3
5–4 550.9263 79.3 HIFI 38.5 0.95 0.75 2.5 11 0.68

Notes. The root-mean square (rms) are expressed in units of main-beam brightness temperature per velocity interval of 1 km s-1. Fluxes are integrated between −140 and −100 km s-1, −90 and −50 km s-1, and −50 and −17 km s-1 for the jet, HH377, and the outflow cavity, respectively. They are expressed in units of main-beam brightness temperature.

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