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Table 1
Correlation between the [C ii] luminosity of the different contributing ISM components and the SFR for different rings in the Galactic plane obtained using BES fits.
| Variable | log SFR = mlog L[ CII ] + b | Dispersion | Spearman’s rank coeff. | Total luminosity | |
| m | b | dex | 1040 erg s-1 | ||
|
|
|||||
| [C ii] Total | 0.98 ± 0.07 | –39.80 ± 2.94 | 0.14 | 0.91 | 10.1 |
| [C ii] (PDRs) | 0.74 ± 0.07 | –30.00 ± 2.81 | 0.12 | 0.88 | 3.2 |
| [C ii] (Electrons) | 0.91 ± 0.06 | –36.30 ± 2.36 | 0.11 | 0.94 | 1.9 |
| [C ii] (HI CNM) | 0.65 ± 0.07 | –26.50 ± 2.75 | 0.14 | 0.86 | 2.5 |
| [C ii] (Dark Gas) | 2.12 ± 0.37 | –84.10 ± 14.30 | 0.21 | 0.84 | 2.5 |
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