Table 3
Detection of line wing emission in high-J CO lines and their comparison to prior outflow detections.
| No. | Source | CO 4−3(a) | CO 6−5(b) | 13CO3−2(c) | 13CO2−1(d) | SiO2−1(e) | CO 11−10(f) | CO 13−12(f) | CO 16−15(f) |
|---|---|---|---|---|---|---|---|---|---|
| 1 | G351.16+0.7 | ✓ | ✓ | … | − | − | ✓ | … | ✓ |
| 2 | G351.25+0.7 | ✓ | ✓ | … | − | − | ✓ | ✓ | ✓ |
| 3 | G351.44+0.7 | ✓ | ✓ | … | − | − | ✓ | … | ✓ |
| 4 | G351.58−0.4 | ✓ | ✓ | … | − | − | ✓ | … | ✓ |
| 5 | G351.77−0.5 | ✓ | ✓ | … | ✓ | − | ✓ | … | ✓ |
| 6 | G12.81−0.2 | ✓ | ✓ | … | ✓ | − | ✓ | ✓ | ✓ |
| 7 | G14.19−0.2 | ✓ | ✓ | … | ✓ | ✓ | ✓ | … | − |
| 8 | G13.66−0.6 | ✓ | ✓ | … | − | ✓ | - | … | − |
| 9 | G14.63−0.6 | ✓ | ✓ | … | − | ✓ | ✓ | … | - |
| 10 | G34.41+0.2 | ✓ | ✓ | − | − | ✓ | ✓ | … | - |
| 11 | G34.26+0.15 | ✓ | ✓ | ✓ | − | ✓ | ✓ | … | ✓ |
| 12 | G34.40-0.2 | ✓ | ✓ | − | − | ✓ | ✓ | … | - |
| 13 | G35.20-0.7 | ✓ | ✓ | − | − | − | ✓ | … | ✓ |
Notes. The symbols have the following meanings: ‘−’ non-detection, ✓ detections, and ‘…’lack of data or unable to detect. (a)Based on single pointing observations from APEX/FLASH+ (Navarete et al. 2019). (b)Obtained from CO 6−5 maps using APEX CHAMP+ (Navarete et al. 2019). (c)Data available only for the sources no. 10−13 in the G34 cloud (Yang et al. 2018a), due to a limited coverage of the CHIMPS survey (Rigby et al. 2016).(d)Based on the identification of line wings towards SEDIGISM sources (Yang etal. 2022). (e)Sources no. 1–5: Mopra molecular lines survey of ATLASGAL sources (Urquhart et al. 2019); and sources no. 6–13: IRAM 30m follow-up of ATLASGAL sources (Csengeri et al. 2016). (f)Wing detection following line decomposition in Sect. 3.2.
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