No molecular emission is seen towards the central space of the half "bs1" (see an arrow in Figure 7b), which may indicate the ionizing influence of large stars related to the S147, S148, and S149 H ii areas. An area of the chosen target complicated is highlighted by a dashed box in Figure 1a. In Figure 1a, the positions of beforehand recognized five H ii areas and SNR G109.1---1.0 (CTB 109) are also marked and labeled. The 5 positions (i.e., p1-p5) are additionally indicated in Figure 7c. Interestingly, these positions are seen toward the overlapping areas of these two cloud parts. In Figure 7c, we've displayed a spatial connection of the two cloud components toward our selected target GMC (see Section 3.2 for extra particulars). Regardless of the location of this material, it remains to be clarified why in these two objects the mud shows properties that deviate so extremely from the standard MW mixture.


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