Fig. 3
APEX/SHeFI spectra (Tmb) of the CO(2–1) (left) and CO(3–2) (right) lines at 230 GHz and 345 GHz, in Haro 11, Mrk 1089, UM 311, and NGC 625 (from top to bottom). The spectra are rebinned to a common resolution of ~10–15 km s-1 (and 3 km s-1 for NGC 625). Central velocities of [C ii], H i, and Hα, and their dispersions are also indicated in blue, green, and red, respectively.
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