Fig. 6.

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Velocity-integrated 12CO intensity (WCO) of two molecular clouds spatially coincident with the direction of LHAASO J2108+5157. Left: Integrated velocity of the first Gaussian component peaking at v1 ≈ −11.8 km s−1, with corresponding distance of d1 ≈ 3.1 kpc. Right: Integral of the second Gaussian component at v2 ≈ −2.7 km s−1 and d1 ≈ 2.0 kpc. The white contour represents 1420 MHz continuum emission from the Canadian Galactic Plane Survey (Taylor et al. 2003). The position of LHAASO J2108+5157 is marked with a black cross, and 95% UL on its extension (0.26°) is indicated with a black circle (Cao et al. 2021a). Bilinear interpolation is used to smooth out the contributions from individual pixels.
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