Draco cloud in HI. Left: channel maps of HI brightness temperature in K from EBHIS at 10′ angular resolution in steps of 4 km s⁻¹. The central velocity is given in the lower-left corner, and the individual velocity components of Draco (high, intermediate, and local) are indicated. Right: zoom into the velocity range of the IVC between −12 and −28 km s⁻¹ using the DRAO with the Synthesis Telescope H I data at 1′ angular resolution (Blagrave et al. 2017) in steps of 0.82 km s⁻¹.