Fig. 2

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Local ISM density evaluation in the direction of the BS. The upper plot shows nup versus nlow. The fitted dashed line follows nup = 16.8 nlow + 2.3. The middle and lower plots show nlow and nup versus the distance above the Galactic plane, z, respectively. The dashed line draws the Dickey & Lockman 1990 and Loup et al. 1993 tendencies. In all the plots, the red points are the stars in the Cygnus X region (1 ~ 79°).
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