ALMA H¹³CN (J = 4–3) and IRTF [Ne II]12.8 μm velocity channel maps from v_LSR = −150 to +150 km s⁻¹ in steps of 10 km s⁻¹. The two top left panels show H¹³CN (J = 4–3) and [Ne II]12.8 μm total integrated line intensity maps. White curves in the H¹³CN (J = 4–3) map represent a CND model bounded by two rotating circular rings (with i = 66°, θ = 23°) with inner and outer deprojected radii of 1.5 and 2.3 pc respectively. Gray curves in the [Ne II]12.8 μm map represent Keplerian elliptical orbits proposed to fit the motion of the ionized gas streamers (Zhao et al. 2009). The other panels show individual H¹³CN velocity channel maps (for intensities between 0 and 20 K km s⁻¹ in linear scale) with the specific velocity interval [v, v + 10] displayed at each corner. The ionized gas emission in the mini-spiral is shown in magenta contours (from Irons et al. 2012). Sgr A^* is at position (0″, 0″) and is displayed with a white dot.