Example of the extent of the emission of H I with the new MeerKAT observations. Top: three-color optical image showing star forming spiral galaxy NGC 1512 and the low-mass dwarf companion NGC 1510 in the optical (image credits: DESI Legacy Survey). The scale bar on the lower left corner indicates 20 kpc. Bottom: same as above but overlaid with H I emission contour levels of log₁₀ 0.25, 1, 1.5, 2, 2.25, 2.5, 2.75, 3 K km s⁻¹ together with the western and southern tidal dwarf galaxies of NGC 1512 (see Section 3 for more information).