Open Access
Fig. A.5
Large-scale spatial distribution of HI emission in the Taurus–Auriga–California–Perseus region from Kalberla et al. (2017). Red, green, and blue are the HI components at the velocity of −29.7 to 3.35, 4.93–8.09, and 8.88–14.41 km s−1. The contour indicates a level of 30 MJy str−1 at the Planck 857 GHz emission.
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