[C I] emission distribution in Haro 11. Upper: distribution of [C I](1–0) emission (color) intensity (left) and velocity (right) contoured with the CO(1–0) emission (black contours), with levels of (1/2)ⁿ (n = 1, 2, …, 8) times of the maximum value of CO intensities. Bottom-left: distribution of the line ratio (R = _1[C I]/I_CO(1−0)) of the [CI] and CO emission intensity. Other symbols are the same as in Fig. 1. Bottom-right: integrated intensity of [C I] pixels versus CO(1–0), in units of mK km s⁻¹. The pixels in Haro 11 are rebinned as ∼0.4″. The average ratios in the disks of spiral galaxies and in (U)LIRGs reported by Jiao et al. (2019) are shown as dotted (R ∼ 0.11) and dashed (R ∼ 0.23) lines, respectively. Black solid lines represent the ratios (R ∼ 0.4–0.6) in the outflow regions that emerge from the nucleus of NGC 253 (Krips et al. 2016).