Table A.1
C2O.
Source | Trans. | ν (a) | Eup (a) | log (Aup /s−1) (a) | Telescope | HPBW | Det. | rms | Tmb | FWHM | Iint | VLSR | Ref. |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
NJ | (MHz) | (K) | (′′) | (mK) | (mK) | (km s−1) | (mK km s−1) | (km s−1) | |||||
C2O | |||||||||||||
TMC-1 | 12 –01 | 22258.2 | 1 | –7.12 | Green Bank-140ft | 79 | Y† | 6 | 1 | ||||
23 –12 | 45 826.7 | 3 | –6.11 | Nobeyama | 41 | Y† | 12 | 1 | |||||
L1544 | 45 –34 | 92 227.9 | 11 | –5.16 | IRAM-ASAI | 27 | Y | 2.4 | 12.8 ± 2.1 | 0.43 ± 0.08 | 5.83 ± 2.04 | 7.12 ± 0.04 | 2 |
44 –33 | 92 363.3 | 11.5 | –5.19 | IRAM-ASAI | 27 | Y | 2.3 | 14.0 ± 2.6 | 0.30 ± 0.07 | 4.45 ± 1.86 | 7.30 ± 0.02 | 2 | |
43 –32 | 92 718.8 | 11 | –5.19 | IRAM-ASAI | 27 | Y | 2.8 | 9.1 ± 2.7 | 0.36 ± 0.12 | 3.47 ± 1.38 | 7.24 ± 0.05 | 2 | |
56 –45 | 115 354.0 | 16.5 | –4.86 | IRAM-ASAI | 22 | N | 16.6 | - | - | - | - | 2 | |
55 –44 | 115 453.0 | 17.1 | –4.88 | IRAM-ASAI | 22 | N | 17.8 | - | - | - | - | 2 | |
54 –43 | 115 656.6 | 16.5 | –4.88 | IRAM-ASAI | 22 | N | 16.8 | - | - | - | - | 2 | |
Elias 18 | 45 –34 | 92 227.9 | 11 | –5.16 | IRAM | 27 | Y | 2.8 | 10.8 ± 2.5 | 0.70 ± 0.19 | 7.99 ± 2.36 | 6.54 ± 0.08 | 2 |
IRAS16293-2422 | 45 –34 | 92 227.9 | 11 | –5.16 | IRAM-TIMASSS | 27 | N | 5 | - | - | - | - | 2 |
L1157-mm | 45 –34 | 92 227.9 | 11 | –5.16 | IRAM-ASAI | 27 | N | 3 | - | - | - | - | 2 |
L1157-B1 | 45 –34 | 92 227.9 | 11 | –5.16 | IRAM-ASAI | 27 | N | 3 | - | - | - | - | 2 |
SVS13A | 45 –34 | 92 227.9 | 11 | –5.16 | IRAM-ASAI | 27 | N | 3 | - | - | - | - | 2 |
OMC-2 FIR4 | 45 –34 | 92 227.9 | 11 | –5.16 | IRAM-ASAI | 27 | N | 3 | - | - | - | - | 2 |
IRAS4A | 45 –34 | 92 227.9 | 11 | –5.16 | IRAM-ASAI | 27 | N | 3 | - | - | - | - | 2 |
Notes. (a) C2O frequencies and spectroscopic parameters were extracted from the Jet Propulsion Laboratory database (JPL; Pickett et al. 1998). † Details of the detection are given in the reference reported in the last column. For the observations towards L1544 the rms on a 50 kHz frequency bin was computed over a range of 15 km s−1. The error in the main-beam temperature Tmb and Iint does not include the 10% calibration accuracy for the IRAM 30 m telescope. Bands with a Tmb value equal to 3σ rms are considered tentative detections, while we attribute the detected status to those bands with a Tmb ≥ 4σ rms.
References. (1) Ohishi et al. (1991), (2) this work.
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