Table 5.
Characteristics of the CO(2-1) and CO(1-0) lines integrated in a 12″ FWHM beam at 3 positions.
| MC13 : Offsets | SCOΔv | V0 | ΔV | Speak | rms | (2–1)/(1–0) |
||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| ID : arcsec | (Jy km s−1) |
(km s−1) |
(km s−1) |
(mJy) |
(mJy) |
Flux | Temp. | |||||
| (2-1) | (1-0) | (2-1) | (1-0) | (2-1) | (1-0) | (2-1) | (1-0) | (2-1) | (1-0) | ratio | ratio | |
| 15 : −9.0,−32.3 | 3.0 ± 0.4 | 1.5 ± 0.3 | −248 ± 2 | −248.0 | 24 ± 4 | 17 ± 3 | 115 | 81 | 16 | 22 | 1.41 | 0.35±0.08 |
| 28 : +15.0,−20.3 | 1.8 ± 0.4 | 1.6±0.3 | −190 ± 1 | −178 | 14 ± 3 | 23 ± 6 | 130 | 64 | 19 | 16 | 2.03 | 0.51 ± 0.15 |
| 36 : +27.0,+3.7 | 4.7 ± 0.8 | 0.91 ± 0.2 | −153 ± 5 | −150.0 | 53 ± 11 | 13 ± 3 | 84 | 68.0 | 20.5 | 17 | 1.23 | 0.31 ± 0.09 |
Notes. The MC13 corresponds to the identification proposed in Melchior & Combes (2013); the offsets of each position are computed with respect to the optical centre. As the parameters, namely integrated flux FCO = SCOΔv, the central velocity V0, linewidth ΔV, peak value Speak, rms level of noise computed on the baseline, and line ratios computed in Jy and in K, are derived from a Gaussian fit in the GILDAS environment.
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