Table 3.
Results from rotational diagram fits in this work.
Molecule | # lines | Trot (K) | Ncol (cm−2) | Zrot | Comments |
---|---|---|---|---|---|
HC5N | 7 | 10.1 ± 0.6 | (4.2 ± 0.4)×1014 | 158.80 | Reliable fit |
HC5N v11 = 1 | 12 | 6.2 ± 1.8 | (7 ± 5)×1012 | 195.20 | Large data dispersion |
H13CCCCCN | 8 | 10.0 ± 1.7 | (9.7 ± 2.7)×1012 | 161.52 | Reliable fit |
HC13CCCCN | 8 | 14.4 ± 2.6 | (8.2 ± 1.7)×1012 | 228.04 | Reliable fit |
HCC13CCCN | 7 | 10.4 ± 1.3 | (1.00 ± 0.19)×1013 | 162.42 | Reliable fit |
HCCC13CCN | 7 | 10.6 ± 1.7 | (1.00 ± 0.25)×1013 | 166.20 | Reliable fit |
HCCCC13CN | 8 | 9.2 ± 0.6 | (1.09 ± 0.13)×1013 | 145.42 | Reliable fit |
HC7N | 17 | 15.8 ± 0.4 | (1.95 ± 0.11)×1014 | 583.44 | Reliable fit |
HC7N v15 = 1 | 31 | 21.3 ± 1.7 | (2.0 ± 0.3)×1013 | 1572.97 | Reliable fit (3 points removed) |
HC7N v15 = 2 | 26 | 12.6 ± 2.5 | (1.0 ± 0.5)×1013 | 1358.51 | Large data dispersion |
H13CCCCCCCN | 11 | 23 ± 4 | (3.0 ± 0.8)×1012 | 879.75 | Reliable fit (1 point removed) |
HC13CCCCCCN | 8 | 15 ± 7 | (3.31 ± 3.41)×1012 | 559.13 | Large data dispersion |
HCC13CCCCCN | 10 | 19 ± 6 | (3.5 ± 2.1)×1012 | 713.79 | Large data dispersion |
HCCC13CCCCN | 10 | 23 ± 4 | (2.7 ± 0.8)×1012 | 836.22 | Reliable fit (2 points removed) |
HCCCC13CCCN | 6 | 16 ± 3 | (3.9 ± 1.7)×1012 | 573.14 | Reliable fit |
HCCCCC13CCN | 11 | 22 ± 6 | (2.7 ± 1.3)×1012 | 824.82 | Large data dispersion |
HCCCCCC13CN | 9 | 31 ± 10 | (3.2 ± 1.1)×1012 | 1156.63 | Reliable fit (1 point removed) |
HC9N | 30 | 22.9 ± 1.1 | (4.5 ± 0.6)×1013 | 1644.03 | Reliable fit (1 point removed) |
HC9N v19 = 1 | 50 | 28.0 ± 2.2 | (2.4 ± 0.4)×1013 | 4009.46 | Reliable fit (1 point removed) |
l-HC4N | 6 | 5.1 ± 2.5 | (3.9 ± 3.7)×1012 | 126.85 | Large data dispersion |
C4H | 4 | 4.9 ± 0.6 | (1.84 ± 0.25)×1014 | 86.42 | Reliable fit |
C4H v7 = 1 | 10 | 10 ± 5 | (6.6 ± 2.0)×1013 | 314.65 | Large data dispersion |
C4H v7 = 2 | 4 | 6.4 ± 1.3 | (2.2 ± 0.4)×1013 | 113.77 | Reliable fit |
C5H 2Π1/2 | 8 | 5.0 ± 0.4 | (2.7 ± 0.5)×1013 | 172.74 | Reliable fit |
C5H 2Π3/2 | 8 | 5.9 ± 0.8 | (2.52 ± 2.48)×1014 | 10.67 | Moderate data dispersion |
C6H 2Π3/2 | 14 | 11.0 ± 0.8 | (1.51 ± 0.14)×1013 | 334.91 | Reliable fit |
C6H 2Π1/2 | 14 | 12.4 ± 0.6 | (1.23 ± 0.18)×1013 | 66.83 | Reliable fit |
C6H v11 = 1 | 14 | 10.4 ± 0.5 | (9.3 ± 0.7)×1012 | 310.61 | Reliable fit (2 points removed) |
C6H 2Δ5/2v11 = 1 | 6 | 13 ± 3 | (2.0 ± 0.5)×1012 | 201.51 | Moderate data dispersion |
C6H 2Δ3/2v11 = 1 | 7 | 21 ± 13 | (1.4 ± 0.7)×1012 | 311.75 | Large data dispersion |
C7H 2Π1/2 | 22 | 13.2 ± 1.4 | (5.1 ± 1.0)×1012 | 1260.39 | Reliable fit (1 point removed) |
C7H 2Π3/2 | 11 | 14.7 ± 2.2 | (3.2 ± 2.0)×1012 | 110.99 | Moderate data dispersion |
C8H 2Π3/2 | 30 | 14.8 ± 0.6 | (8.9 ± 0.9)×1012 | 2111.08 | Reliable fit (1 point removed) |
C8H 2Π1/2 | 16 | 8.0 ± 1.4 | (1.15 ± 1.38)×1013 | 35.16 | Large data dispersion |
C5N− | 6 | 8.8 ± 1.4 | (4.9 ± 1.6)×1012 | 132.62 | Reliable fit |
C6H− | 7 | 11.4 ± 1.0 | (4.3 ± 0.6)×1012 | 173.51 | Reliable fit |
C8H− | 13 | 23 ± 5 | (1.1 ± 0.4)×1012 | 810.24 | Reasonable fit. Large data dispersion |
SiC4 | 6 | 12.9 ± 1.8 | (6.2 ± 1.0)×1012 | 175.36 | Reliable fit |
29SiC4 | 5 | 10 ± 6 | (5.73 ± 5.06)×1011 | 134.88 | Large data dispersion |
SiC6 | 7 | 17.3 ± 2.5 | (1.3 ± 0.4)×1012 | 588.57 | Reliable fit (1 point removed) |
CCS | 4 | 7.9 ± 1.1 | (4.0 ± 0.7)×1013 | 44.48 | Reliable fit |
C3S | 3 | 23.60 ± 96.85 | (2.58 ± 3.60)×1013 | 170.50 | Very high data dispersion |
NaCN | 7 | 24 ± 13 | (8.5 ± 1.7)×1012 | 425.76 | Large data dispersion (1 point removed) |
MgC3N | 14 | 11.1 ± 0.9 | (5.2 ± 0.6)×1012 | 336.00 | Reliable fit (1 point removed) |
MgC5N | 30 | 15.4 ± 1.8 | (4.7 ± 1.3)×1012 | 1109.27 | Reliable fit (1 point removed) |
MgC4H | 10 | 4.7 ± 1.2 | (1.5 ± 1.3)×1013 | 140.43 | Large data dispersion |
MgC6H | 30 | 24.8 ± 8.9 | (2.0 ± 0.9)×1013 | 966.24 | Large data dispersion |
Notes. Trot: Rotational temperature. Ncol: Column density. Zrot: Partition function. The resulting fits are plotted in Fig. 4 on top of the data points we used for the fits (extracted from the individual line fits as listed in Table A.1). Species with unreliable fits due to a very low number of data points or extremely high data dispersion in them, are not shown. These species, and others with a very low number of detected lines here, will be revisited in future publications of similar 4.3 to 1.0 mm surveys carried out with the IRAM-30m telescope.
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