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2017

Croxall, Kevin, Smith, J. D. T., Pellegrini, Eric et al.

The [CII] 158um fine-structure line is the brightest emission line observed in local star-forming galaxies.

As a major coolant of the gas-phase interstellar medium, [CII] balances the heating, including that due to far-ultraviolet photons, which heat the gas via the photoelectric effect.
However, the origin of [CII] emission remains unclear, because C+ can be found in multiple phases of the interstellar medium.
Here we measure the fractions of [CII] emission originating in the ionized and neutral gas phases of a sample of nearby galaxies.

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