Smirnova-Pinchukova, I.; Husemann, B.; Busch, G.; Appleton, P.; Bethermin, M.; Combes, F.; Croom, S.; Davis, T. A.; Fischer, C.; Gaspari, M.; Groves, B.; Klein, R.; O'Dea, C. P.; Pérez-Torres, M.; Scharwächter, J.; Singha, M.; Tremblay, Grant R.; Urrutia, T.
(2019)
The [C II]?158 µm line is one of the strongest far-infrared (FIR) lines and an important coolant in the interstellar medium of galaxies that is accessible out to high redshifts. The excitation of [C II] is complex and can ...
