to further explore various cloud components. In Figure \[fig4\]c, we display the observed $^{13}$CO(J =1$-$0) and C$^{18}$O(J =1$-$0) spectra in the direction of an area highlighted by a solid box in Figure \[fig4\]a), revealing two noticeable velocity peaks (i.e., 35 and 53 km s$^{-1}$). These profiles are produced by averaging the selected area.

In the direction of the selected target area, Figures \[fig5\]a and \[fig5\]b display the integrated $^{13}$CO (J=1–0) and C$^{18}$O (J=1–0) intensity maps, respectively. In each intensity map, the molecular gas is integrated over a velocity range of \[29.6, 60.2\] km s$^{-1}$. Both the maps display an extended morphology of the molecular cloud associated with the selected target area, appearing like a giant molecular cloud (GMC). .

Figure \[fig6\] presents the integrated $^{13}$CO velocity channel maps (at intervals of 1.3 km s$^{-1}$). The distribution of $^{13}$CO gas in the channel maps suggests the existence of different velocity components in the direction of the selected physical system (see panels at \[36.82, 38.12\], \[44.62, 45.92\], and \[53.72, 55.02\] km s$^{-1}$). In Figures \[fig7\]a and \[fig7\]b, we show the longitude-velocity maps of $^{13}$CO and C$^{18}$O, respectively. Both the position-velocity maps depict three velocity components around 35, 45, and 53 km s$^{-1}$ 