The nature of the [C ii] emission in dusty star-forming galaxies from the SPT survey

• Published in: Monthly Notices of the Royal Astronomical Society
• Main Authors: Gullberg, B., Murphy, E. J.
• Format: Article in Journal/Newspaper
• Language: English
• Published: Royal Astronomical Society 2015
• Subjects: South Pole; South pole
• Online Access: https://authors.library.caltech.edu/58608/; https://authors.library.caltech.edu/58608/1/MNRAS-2015-Gullberg-2883-900.pdf; https://authors.library.caltech.edu/58608/2/1501.06909v2.pdf; https://resolver.caltech.edu/CaltechAUTHORS:20150625-115259135

We present [C ii] observations of 20 strongly lensed dusty star-forming galaxies at 2.1 < z < 5.7 using Atacama Pathfinder EXperiment and Herschel. The sources were selected on their 1.4 mm flux (S1.4 mm > 20 mJy) from the South Pole Telescope (SPT) survey, with far-infrared (FIR) luminosities determined from extensive photometric data. The [C ii] line is robustly detected in 17 sources, all but one being spectrally resolved. 11 out of 20 sources observed in [C ii] also have low-J CO detections from Australia Telescope Compact Array. A comparison with mid- and high-J CO lines from Atacama Large Millimeter/submillimeter Array reveals consistent [C ii] and CO velocity profiles, suggesting that there is little differential lensing between these species. The [C ii], low-J CO and FIR data allow us to constrain the properties of the interstellar medium. We find [C ii] to CO(1–0) luminosity ratios in the SPT sample of 5200 ± 1800, with significantly less scatter than in other samples. This line ratio can be best described by a medium of [C ii] and CO emitting gas with a higher [C ii] than CO excitation temperature, high CO optical depth τ_CO(1–0) ≫ 1, and low to moderate [C ii] optical depth τ_[CII]≲ 1. The geometric structure of photodissociation regions allows for such conditions.