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Using the Purple Mountain Observatory Delingha (PMODLH) 13.7 m telescope, wereport a 96-square-degree 12CO/13CO/C18O mapping observation toward theGalactic region of l = [139.75, 149.75]$^\circ$, b = [-5.25, 5.25]$^\circ$. Themolecular structure of the Local Arm and Perseus Arm are presented. CombiningHI data and part of the Outer Arm results, we obtain that the warp structure ofboth atomic and molecular gas is obvious, while the flare structure only existsin atomic gas in this observing region. In addition, five filamentary giantmolecular clouds on the Perseus Arm are identified. Among them, four are newlyidentified. Their relations with the Milky Way large-scale structure arediscussed.

The Molecular Structures of Local Arm and Perseus Arm in the Galactic Region of l=[139.75,149.75]$^\circ$, b=[-5.25,5.25]$^\circ$