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Fig. 5

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Integrated 12CO (J = 1–0) emission intensity (K km s−1) toward γ-Cygni region in the velocity ranges [+9.0, +12.0] km s−1 (left panel) and [−16.0, −11.0] km s−1 (right panel) using MWISP data. The solid circles are the same as in Figure 3. The dashed magenta and red circles correspond to different regions that are affected by escaped CRs, called CloudV and CloudH, respectively.

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