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تسجيل مستخدم جديدThe Molecular Clouds associated with the H II Regions/Candidates between $l=207.7^circ$ and $l=211.7^circ$
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Using the PMO-13.7 m millimeter telescope at Delingha in China, we have conducted a large-scale simultaneous survey of $^{12}$CO, $^{13}$CO, and C$^{18}$O $J=1-0$ emission toward the sky region centered at $l$=$209.7^circ$, $b$=$-$2.25$^circ$ with a coverage of $4.0^circ times 4.5^circ$. The majority of the emission in the region comes from the clouds with velocities lying in the range from $-$3 km s$^{-1}$ to 55 km s$^{-1}$, at kinematic distances from 0.5 kpc to 7.0 kpc. The molecular clouds in the region are concentrated into three velocity ranges. The molecular clouds associated with the ten H II regions/candidates are identified and their physical properties are presented. Massive stars are found within Sh2-280, Sh2-282, Sh2-283, and BFS54, and we suggest them to be the candidate excitation sources of the H II regions. The distributions of excitation temperature and line width with the projected distance from the center of H II region/candidate suggest that the majority of the ten H II regions/candidates and their associated molecular gas are three-dimensional structures, rather than two-dimensional structures.
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We have studied the properties of molecular clouds in the second quadrant of the Milky Way Mid-plane from l$=$104$.!!^{circ}$75 to l$=$119$.!!^{circ}$75 and b$=-$5$.!!^{circ}$25 to b$=$5$.!!^{circ}$25 using the $^{12}$CO, $^{13}$CO, and C$^{18}$O $J=
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