Fig. 1

Maps of the Cetus (Cet), Main Taurus (TauM), South Taurus (TauS), North Taurus (TauN), Perseus (Per), and California (Cal) clouds, and of the Galactic disc background (Gal) in H icolumn density, NHI, for a spin temperature of 400 K, and in CO intensity, WCO. The NHI and WCO maps are respectively labelled HI and CO. The map labelled ff shows the intensity Iff of free-free emission toward this region. The last subplot shows the coverage of the GALFA (dark grey) and EBHIS (light blue) H i data.
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