2014ApJ...787....8R

We report on two regularly rotating galaxies at redshift z ~ 2, using high-resolution spectra of the bright [C II] 158 µm emission line from the HIFI instrument on the Herschel Space Observatory. Both SDSS090122.37+181432.3 ("S0901") and SDSSJ120602.09+514229.5 ("the Clone") are strongly lensed and show the double-horned line profile that is typical of rotating gas disks. Using a parametric disk model to fit the emission line profiles, we find that S0901 has a rotation speed of vsin (i) ~ 120±7 km/s and a gas velocity dispersion of σ_g< 23 km/s (1σ). The best-fitting model for the Clone is a rotationally supported disk having vsin (i) ~ 79±11 km/s and σ_g ≲ 4 km/s (1σ). However, the Clone is also consistent with a family of dispersion-dominated models having σ_g= 92±20 km/s. Our results showcase the potential of the [C II] line as a kinematic probe of high-redshift galaxy dynamics: [C II] is bright, accessible to heterodyne receivers with exquisite velocity resolution, and traces dense star-forming interstellar gas. Future [C II] line observations with ALMA would offer the further advantage of spatial resolution, allowing a clearer separation between rotation and velocity dispersion.