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• W2311635880 abstract "Observations of ionised carbon at 158 micron ([CII]) from luminous star-forming galaxies at z~0 show that their ratios of [CII] to far infrared (FIR) luminosity are systematically lower than those of more modestly star-forming galaxies. In this paper, we provide a theory for the origin of this so called [CII] deficit in galaxies. Our model treats the interstellar medium as a collection of clouds with radially-stratified chemical and thermal properties, which are dictated by the clouds' volume and surface densities, as well as the interstellar radiation and cosmic ray fields to which they are exposed. [CII] emission arises from the outer, HI dominated layers of clouds, and from regions where the hydrogen is H2 but the carbon is predominantly C+. In contrast, the most shielded regions of clouds are dominated by CO and produce little [CII] emission. This provides a natural mechanism to explain the observed [CII]-star formation relation: galaxies' star formation rates are largely driven by the surface densities of their clouds. As this rises, so does the fraction of gas in the CO-dominated phase that produces little [CII] emission. Our model further suggests that the apparent offset in the [CII]-FIR relation for high-z sources compared to those at present epoch may arise from systematically larger gas masses at early times: a galaxy with a large gas mass can sustain a high star formation rate even with relatively modest surface density, allowing copious [CII] emission to coexist with rapid star formation." @default.
• W2311635880 created "2016-06-24" @default.
• W2311635880 creator A5014544028 @default.
• W2311635880 creator A5057320280 @default.
• W2311635880 date "2016-12-10" @default.
• W2311635880 modified "2023-09-27" @default.
• W2311635880 title "A physical model for the [C ii]–FIR deficit in luminous galaxies" @default.
• W2311635880 cites W1518747726 @default.
• W2311635880 cites W1524555145 @default.
• W2311635880 cites W1623182580 @default.
• W2311635880 cites W1653633141 @default.
• W2311635880 cites W1844053863 @default.
• W2311635880 cites W1851199749 @default.
• W2311635880 cites W1866562585 @default.
• W2311635880 cites W1918040529 @default.
• W2311635880 cites W1925665838 @default.
• W2311635880 cites W1931688456 @default.
• W2311635880 cites W1946983611 @default.
• W2311635880 cites W1965120300 @default.
• W2311635880 cites W1972016247 @default.
• W2311635880 cites W1973168596 @default.
• W2311635880 cites W1975557117 @default.
• W2311635880 cites W1978081588 @default.
• W2311635880 cites W1979348280 @default.
• W2311635880 cites W1982453941 @default.
• W2311635880 cites W1983324871 @default.
• W2311635880 cites W1984072856 @default.
• W2311635880 cites W1987477766 @default.
• W2311635880 cites W1987821954 @default.
• W2311635880 cites W1994821728 @default.
• W2311635880 cites W1997662069 @default.
• W2311635880 cites W1997824835 @default.
• W2311635880 cites W1998859910 @default.
• W2311635880 cites W2001268331 @default.
• W2311635880 cites W2004052728 @default.
• W2311635880 cites W2006391693 @default.
• W2311635880 cites W2006878995 @default.
• W2311635880 cites W2006951810 @default.
• W2311635880 cites W2016752210 @default.
• W2311635880 cites W2023793647 @default.
• W2311635880 cites W2024626682 @default.
• W2311635880 cites W2025105301 @default.
• W2311635880 cites W2025152207 @default.
• W2311635880 cites W2031622689 @default.
• W2311635880 cites W2031741356 @default.
• W2311635880 cites W2032832347 @default.
• W2311635880 cites W2033995141 @default.
• W2311635880 cites W2044043297 @default.
• W2311635880 cites W2044486458 @default.
• W2311635880 cites W2047156688 @default.
• W2311635880 cites W2049698250 @default.
• W2311635880 cites W2058484847 @default.
• W2311635880 cites W2058746963 @default.
• W2311635880 cites W2060850421 @default.
• W2311635880 cites W2066265110 @default.
• W2311635880 cites W2066835107 @default.
• W2311635880 cites W2069524830 @default.
• W2311635880 cites W2070716474 @default.
• W2311635880 cites W2071884317 @default.
• W2311635880 cites W2075090561 @default.
• W2311635880 cites W2075770183 @default.
• W2311635880 cites W2076955670 @default.
• W2311635880 cites W2085713960 @default.
• W2311635880 cites W2086140797 @default.
• W2311635880 cites W2088763329 @default.
• W2311635880 cites W2088892484 @default.
• W2311635880 cites W2093835827 @default.
• W2311635880 cites W2094504621 @default.
• W2311635880 cites W2095757078 @default.
• W2311635880 cites W2102080842 @default.
• W2311635880 cites W2109222834 @default.
• W2311635880 cites W2119238619 @default.
• W2311635880 cites W2121404382 @default.
• W2311635880 cites W2123048580 @default.
• W2311635880 cites W2123091654 @default.
• W2311635880 cites W2123267088 @default.
• W2311635880 cites W2127065577 @default.
• W2311635880 cites W2131276156 @default.
• W2311635880 cites W2138093180 @default.
• W2311635880 cites W2140347367 @default.
• W2311635880 cites W2140888726 @default.
• W2311635880 cites W2142779957 @default.
• W2311635880 cites W2146026248 @default.
• W2311635880 cites W2148031907 @default.
• W2311635880 cites W2150550921 @default.
• W2311635880 cites W2154230608 @default.
• W2311635880 cites W2165672197 @default.
• W2311635880 cites W2168900818 @default.
• W2311635880 cites W2169039585 @default.
• W2311635880 cites W2171942739 @default.
• W2311635880 cites W2197630840 @default.
• W2311635880 cites W2256626468 @default.
• W2311635880 cites W2511877802 @default.
• W2311635880 cites W2599301852 @default.
• W2311635880 cites W2600822636 @default.
• W2311635880 cites W2949460745 @default.
• W2311635880 cites W2952264677 @default.
• W2311635880 cites W2952520614 @default.

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