Table 5
Physical conditions and cosmic ray ionisation rates.
Pos. | Δv | nH2 | Tkin | N(C18O) | AV | N(H13CO+) | N(DCO+) |
![]() |
ζ |
[ km s-1] | [103 cm-3] | [K] | [1015 cm-2] | [mag] | [1012 cm-2] | [1012 cm-2] | [10-17 s-1] | ||
|
|||||||||
N1 | 3.5 | 0.6 {0.2−1} | 15 ± 5 | 4 {2−6} | 21 {11−32} | 0.8−1.3 | <0.22 | <0.005 | >13 |
N5 | 3.0 | 4 {2−5} | 10 ± 2 | 3 {2−8} | 16 {11−32} | 1.1−1.4 | 0.89−1.30 | 0.014−0.020 | 130−330 |
N6 | 3.0 | 4 {2−6} | 13 ± 3 | 6 {4−20} | 32 {21−105} | 1.8−2.5 | 0.79−1.30 | 0.008−0.012 | 130−400 |
N2 | 5.0 | > 2 | 16 ± 2 | 20 {15−30} | 105 {79−158} | 5.6−8.9 | 1.10−2.00 | 0.003−0.006 | − |
N7 | 2.5 | 2 {2−5} | 10 ± 2 | 4 {3−10} | 21 {16−53} | 0.6−0.9 | <0.25 | <0.007 | >130 |
N8 | 3.5 | 1 {0.6−2} | 8 ± 1 | 3 {2−4} | 16 {11−21} | <0.2 | <0.35 | − | − |
N3 | 3.5 | 6 {4−10} | 8 ± 1 | 6 {5−7} | 32 {26−37} | 1.0−1.4 | <0.35 | <0.006 | >260 |
N4 | 3.0 | 2 {0.6−4} | 12 ± 3 | 2 {2−3} | 11 {5−16} | 1.0−1.4 | <0.35 | <0.006 | >40 |
SE1 | 4.0 | 2 {1−5} | 19 ± 5 | 6 {5−20} | 32 {26−105} | 0.4−0.56 | 0.79−1.0 | 0.032−0.05 | 0.2−20 |
SE2 | 3.0 | 4 {2−10} | 8 ± 2 | 0.9 {0.4−20} | 5 {2−105} | <0.2 | <0.28 | − | − |
SW2 | 1.5 | 2 {1−4} | 20 ± 4 | 4 {3−10} | 21 {16−53} | <0.1 | <0.22 | − | − |
SW4† | 1.5 | 6 {4−10} | 16 ± 2 | 1.5 {1−3} | 5 {5−16} | 0.5−0.8 | <0.25 | <0.009 | − |
Notes. nH2 is the molecular hydrogen density (cm-3), Tkin the gas kinetic temperature, N(C18O) the total column density of C18O. AV is the visual extinction assuming [C18O] = AV × 1.9 1014 cm-2 (Frerking et al. 1982; Bolatto et al. 2013). We assumed isotopic ratio values 18O /16O = 500 and 13C /12C = 50 (see text). Values in brackets indicate the range of values satisfying . Uncertainties on nH2 and Tkin are at the 70% confidence level, and are propagated in the abundance ratios and upper limits. Lower limits of ζ were deduced from chemical modelling (see Sect. 6).
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