Table 6
Logarithm of the measured ISM column densities (in cm-2).
| LS III +46 11 | LS III +46 12 | |||||
| Line(s) | St. comp. | Wk. comp. | Total | St. comp. | Wk. comp. | Total |
| CN λ3873.999+74.607+75.760 | 12.98±0.05 | 11.99±0.06 | ||||
| CH+ λ3957.692 | 13.79±0.03 | 13.83±0.07 | ||||
| Ca iλ4226.7275 | 10.70±0.04 | 10.76±0.08 | ||||
| CH+ λ4232.548 | 13.73±0.02 | 13.25±0.20 | 13.85±0.02 | 13.89±0.05 | ||
| CH λ4300.313 | 13.99±0.02 | 13.19±0.08 | 14.05±0.02 | 13.74±0.05 | ||
| K iλ7664.911+7698.974 | 12.40±0.01 | 11.84±0.04 | 12.50±0.02 | 12.23±0.01 | 11.85±0.03 | 12.38±0.02 |
Notes. When high-resolution spectra are available, the column densities for the two components plus the total value are given using the kinematic decomposition described in the text. In the other cases, we used the EWs from Tables 2 and 4. Since for CH+ λ4232.548 and CH λ4300.313 no high-resolution spectra were available for LS III +46 12 and those lines have a slight saturation effect, we applied a correction to the EW based on the comparison between the intermediate-resolution and high-resolution results for those lines in LS III +46 11. The molecular oscillator strengths used are those of Smoker et al. (2014), while those for the atomic lines were obtained from the NIST web page http://physics.nist.gov/Pubs/AtSpec/table105.html/.
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