Table B.7
Peak main beam temperatures for 13CO.
| System | 3–2a | 4–3b | 6–5b | 10–9c | ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Tmb | Noise | Width | Integrated | Tmb | Noise | Width | Integrated | Tmb | Noise | Width | Integrated | Tmb | Noise | Width | Integrated | |
| K | K | km s−1 | K km s−1 | K | K | km s−1 | K km s−1 | K | K | km s−1 | K km s−1 | K | K | km s−1 | K km s−1 | |
| Wide multiples | ||||||||||||||||
| L1448N | 7.51 | 0.12 | 2.15 | 17.22 | 1.95 | 0.49 | 2.03 | 4.22 | 0.30 | 0.03 | 1.0034 | |||||
| SVS 13-A | 4.83 | 0.56 | 1.71 | 8.78 | ||||||||||||
| SVS 13-C | 4.66 | 0.50 | 1.57 | 7.78 | ||||||||||||
| IRAS 7d | 7.20 | 0.13 | 2.93 | 22.46 | 3.44 | 0.14 | 1.41 | 5.16 | 0.11 | 0.03 | 0.17 | |||||
| B1-B | … | 0.19 | … | … | ||||||||||||
| PER8+PER55 | 8.05 | 0.12 | 2.48 | 21.23 | 2.51 | 0.06 | 2.07 | 5.54 | 0.18 | 0.03 | 0.6882 | |||||
| Close binaries | ||||||||||||||||
| IRAS 1 | 5.47 | 0.13 | 1.40 | 8.16 | 1.57 | 0.33 | 1.10 | 1.84 | 0.11 | 0.03 | 0.2244 | |||||
| IRAS 03282 | 1.99 | 0.75 | 0.62 | 1.32 | … | 0.40 | … | … | … | 0.03 | … | … | ||||
| IRAS 03292 | 3.26 | 0.44 | 0.84 | 2.91 | … | 0.12 | … | … | … | 0.03 | … | … | ||||
| Singles | ||||||||||||||||
| IRAS 03271 | 3.85 | 0.13 | 1.06 | 4.35 | … | 0.37 | … | … | 0.09 | 0.03 | … | … | ||||
| Per25 | … | 0.42 | … | … | … | 0.03 | … | … | ||||||||
| SK1 | 4.47 | 0.13 | 2.26 | 10.73 | … | 0.29 | … | … | … | 0.03 | … | … | ||||
Notes. Blank spaces indicate that there are no observations for the respective system and transition; three dots (…) indicate non-detection. (a)Peak antenna temperatures from JCMT observations, smoothed to a beam of 19.25′′. (b)Peak antenna temperatures and noise from APEX observations, averaged over a box of 19.25′′. (c) Peak antenna temperatures from Herschel HIFI observations with a beam of 19.25′′ (Mottram et al. 2017). (d)IRAS 7 here includes only Per18 and Per21.
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