Table 5
Molecular line emission from the CCS componenta.
| Line | Apertureb | S | Δυc | I | Sized |
|---|---|---|---|---|---|
| (′′) | (Jy) | (km s−1) | (Jy km s−1) | ||
| CO(2–1) | 0.2 | 0.15 | 18.7 | 3.0 | 0.′′15 |
| 13CO(2–1) | 0.6 | 0.35 | 6.2 | 2.3 | … |
| C18O(2–1) | 0.6 | 0.20 | 2.9 | 0.61 | … |
| 13C17O(2–1)e | 0.6 | 0.015 | 3.7 | 0.059 | |
| SiO(5–4) | 0.2 | 0.046 | 11.9 | 0.58 | 0.′′10 |
| 29SiO(5–4) | 0.2 | 0.013 | 10.0 | 0.14 | 0.′′11 |
| SiS(12–11)e | 0.6 | 0.011 | 3.3 | 0.038 | … |
| SiS(13–12)e | 0.6 | 0.010 | 4.2 | 0.045 | … |
| 13CS(5–4)e | 0.6 | 0.027 | 2.5 | 0.072 | … |
| SO(55 − 44) | 0.2 | 0.073 | 4.4 | 0.34 | 0.′′15 |
| SO(56 − 45) | 0.6 | 0.10 | 3.7 | 0.41 | … |
| SO(65 − 54)f | 25 | 0.22 | 5.1 | 1.2 | … |
| SO(87 − 77) | 0.2 | 0.011 | 2.5 | 0.029 | … |
| 33SO(56–45)g | 0.6 | … | … | 0.019 | … |
| 34SO(56–45) | 0.2 | 0.025 | 2.7 | 0.072 | 0.′′19 |
| SO2(422–313) | 0.6 | 0.043 | 2.3 | 0.11 | … |
| SO2(161,15–152,14) | 0.6 | 0.043 | 2.2 | 0.10 | … |
| SO2(163,13–162,14) | 0.2 | 0.025 | 2.6 | 0.069 | 0.′′17 |
| SO2(222,20–221,21) | 0.2 | 0.015 | 3.2 | 0.051 | 0.′′15 |
| SO2(283,25–282,26) | 0.6 | 0.019 | 1.8 | 0.036 | … |
| OCS(19–18) | 0.2 | 0.023 | 3.2 | 0.078 | 0.′′14 |
| p-H2S(220–211) | 0.2 | 0.084 | 3.6 | 0.32 | 0.′′15 |
p-H S(220–211)g |
0.2 | … | … | 0.15 | … |
p-H S(220–211) |
0.2 | 0.060 | 2.9 | 0.18 | 0.′′26 |
Notes. (a) See Sect. 3 for a discussion ofthe flux uncertainties. (b)The choice of aperture reflects the angular resolution of the ALMA data: the resolutions are ≈0.′′085 and ≈0.′′55 at 0.′′ 2 and 0.′′ 6 aperture, respectively. The apertures are centred on the continuum peak. (c) FWHM of Gaussian fit to the line within the given aperture at 1.5 km s−1 resolution. (d)Mean of the deconvolved FWHMs of a 2D Gaussian fit to the high-angular-resolution ALMA data. (e) These emissions are patchy and extended over a region of ≈0.′′5. (f) This is based on APEX data and the split into emission from the CCS and EDE components obtained using Gaussian decomposition is uncertain. (g) The integrated intensity of the sum of the hyperfine components.
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