Table A.2
Base-ten logarithm of molecular abundances in Galactic and extragalactic sources.
| NGC 4418 | Arp220 | M 82 | NGC 253 | NGC 1068 | SgrB2(N) | SgrB2(OH) | Orion Bar | TMC-1 | PKS1830 | |
|
|
||||||||||
| SiO | –9.2...–8.2 | –9.4...–8.9 | – | –10.2...–10.0 | –9.5...–9.3 | –10.9...–10.3 | – | –10.4...–10.2 | <–11.6 | –9.5...–9.3 |
| H2S | –7.8...–6.7 | –7.0...–6.7 | –9.6...–8.5 | –9.5...–9.1 | – | –10.2...–9.5 | – | –8.3...–8.1 | <–9.3 | – |
| c-HCCCH | –7.8...–6.7 | –8.6...–8.2 | –9.3...–8.8 | –9.4...–9.1 | –10.1...–9.8 | –11.0...–9.9 | –10.4...–9.5 | –9.8...–9.6 | –9.4...–9.2 | –8.7...–8.5 |
| HC3N | –8.5...–7.2 | –8.0...–7.7 | –9.7...–8.9 | –9.7...–9.3 | –8.9...–8.1 | –7.8...–7.0 | –9.5...–8.9 | – | –8.3...–8.1 | –9.4...–9.2 |
| NH2CN | –9.0...–8.0 | – | –9.9...–9.0 | –10.0...–9.5 | <–9.7 | –11.1...–9.6 | –10.4...–9.4 | – | – | – |
| CH3CN | –8.4...–7.6 | –8.5...–8.1 | –10.2...–9.6 | –9.7...–9.3 | –9.6...–9.5 | –7.0...–6.2 | –9.9...–9.3 | <–10.3 | –9.1...–8.9 | –9.3...–9.1 |
| CH3OH | –8.5...–7.4 | –7.7...–7.2 | –9.6...–8.2 | –7.9...–7.7 | –7.9...–7.7 | –6.1...–5.4 | –8.3...–7.2 | <–10.1 | –8.8...–8.6 | –8.2...–8.0 |
| H2CO | –8.3...–7.5 | –8.9...–8.5 | –8.9...–8.4 | –9.0...–8.7 | <–7.1 | –9.6...–8.9 | –8.3...–7.6 | –8.3...–8.1 | –7.8...–7.6 | –8.0...–7.8 |
| CH3CCH | –7.8...–6.7 | –7.5...–7.1 | –7.8...–7.4 | –8.2...–8.0 | <–8.5 | –8.6...–7.9 | –9.1...–8.4 | <–8.5 | –8.3...–8.1 | –8.6...–8.4 |
Notes. For NGC 4418, the range of values represents the confidence interval of the χ2 minimization in the best fit model. Data for Sgr B2(N), Sgr B2(OH), the Orion Bar, TMC-1, and NGC 253 were taken from Martín et al. (2006). Data for Arp 220, NGC 1068, and PKS 1830-211, were taken from Martín et al. (2011), Aladro et al. (2013), and Muller et al. (2011) respectively.
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