Moment-zero and combined channel maps at different dv for two different configurations. Here, the selected channels are the ones where the gas emission is located closest to the planet in order to clearly see its impact on the gas. In the first top rows, a Jupiter-mass planet located at 50 AU is hosted in a 10⁻³ M_⊕ disk, producing a gap; while in the two last rows, a Jupiter mass planet located at 100 AU is introduced in a more massive disk (10⁻¹ M_⊕), producing a kink. The disks are located at 40 pc and are inclined with increasing inclination from left (i = 10°) to right (i = 80°). The visibility of the kink (traced by the red circle) is highly influenced by the disk’s inclination, unlike the gaps.