A Herschel/PACS Far-infrared Line Emission Survey of Local Luminous Infrared Galaxies
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![Table 1 presents the measurements, made available in electronic form, for each line ([ ]OI 63 , [O III ] 88 , [N II ] 122 , and [ C II ] 158 )](https://thumb-us.123doks.com/thumbv2/123dok_us/8234116.2182668/4.918.476.855.112.374/table-presents-measurements-available-electronic-form-line-iii.webp)
![Figure 1. Line de ficits of the [O I ] 63.2 μm, [O III ] 88.4 μm, [N II ] 121.9 μm, [C II ] 157.7 μm, and [N II ] 205.2 μm emission lines, defined as the line-to](https://thumb-us.123doks.com/thumbv2/123dok_us/8234116.2182668/7.918.103.820.75.895/figure-line-ficits-iii-emission-lines-defined-line.webp)
![Figure 2. Line de ficits of the [ ] O I 63 , [O III ] 88 , [N II ] 122 , [ C II ] 158 , and [N II ] 205 emission lines, de fined as the ratio of line luminosity to L IR 8 1000 m [ – m ] as a function of the IR luminosity surface density, de fined as S IR =(](https://thumb-us.123doks.com/thumbv2/123dok_us/8234116.2182668/9.918.98.823.74.889/figure-ficits-emission-luminosity-function-luminosity-surface-density.webp)
![Figure 3. Fraction of PDR contribution to the total [ C II ] 158 emission,](https://thumb-us.123doks.com/thumbv2/123dok_us/8234116.2182668/10.918.64.443.114.238/figure-fraction-pdr-contribution-total-c-ii-emission.webp)
![Figure 5. The quantities shown in the y-axes of all panels, [ C II ] 158 ion /FIR (top left), [ C II ] 158 /FIR/[ C II ] 158 ion -fit (top right), and [ C II ] 158 /FIR (bottom), are presented as a function of the FIR S 63 /S 158 continuum ratio for the ent](https://thumb-us.123doks.com/thumbv2/123dok_us/8234116.2182668/12.918.96.823.76.729/figure-quantities-shown-panels-presented-function-continuum-ratio.webp)
![Figure 6. [ O I ] 63 /[ C II ] 158 PDR ratio as a function of the FIR S 63 /S 158 continuum ratio for the entire GOALS sample (open circles) and the ULIRGs from Farrah et al](https://thumb-us.123doks.com/thumbv2/123dok_us/8234116.2182668/13.918.71.436.78.351/figure-function-continuum-entire-goals-circles-ulirgs-farrah.webp)
![Figure 7. Herschel /PACS spectra (black line) of the five galaxies with [ ] O I 63 /[ C II ] 158 PDR ratios lower than half the value of the fit to the correlation in Figure 6 (dot- (dot-dashed line) that show clear signs of absorption in their [ ]OI 63 line](https://thumb-us.123doks.com/thumbv2/123dok_us/8234116.2182668/14.918.95.821.72.1012/figure-herschel-spectra-galaxies-ratios-correlation-figure-absorption.webp)
![Figure 8. [O III ] 88 /[ ] O I 63 ratio as a function of the FIR S 63 /S 158 ratio for the GOALS sample with available measurements of the lines (open circles), and the DGS from Cormier et al](https://thumb-us.123doks.com/thumbv2/123dok_us/8234116.2182668/15.918.72.436.78.350/figure-function-goals-sample-available-measurements-circles-cormier.webp)
![Figure 9. [O III ] 88 /[N II ] 122 ratio as a function of the [Ne III ] 15.6 /[Ne II ] 12.8 ratio for the GOALS sample (red filled circles)](https://thumb-us.123doks.com/thumbv2/123dok_us/8234116.2182668/16.918.72.435.75.353/figure-ratio-function-ratio-goals-sample-filled-circles.webp)
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