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We have carried out a new kinematical analysis of the molecular gas in theSh2-233 region by using the CO $J$ = 2-1 data taken at $\sim$0.5 pc resolution.The molecular gas consists of a filamentary cloud of 5-pc length with 1.5-pcwidth where two dense cloud cores are embedded. The filament lies between twoclouds, which have a velocity difference of 2.6 km s$^{-1}$ and are extendedover $\sim$5 pc. We frame a scenario that the two clouds are colliding witheach other and compressed the gas between them to form the filament in$\sim$0.5 Myr which is perpendicular to the collision. It is likely that thecollision formed not only the filamentary cloud but also the two dense cores.One of the dense cores is associated with the high-mass protostellar candidateIRAS 05358+3543, a representative high-mass protostar. In the monolithiccollapse scheme of high mass star formation, a compact dense core of 100$M_\odot$ within a volume of 0.1 pc radius is assumed as the initial condition,whereas the formation of such a core remained unexplained in the previousworks. We argue that the proposed collision is a step which efficientlycollects the gas of 100 $M_\odot$ into 0.1 pc radius. This lends support forthat the cloud-cloud collision is an essential process in forming the compacthigh-mass dense core, IRAS 05358+3543.

Evidence for a Cloud-Cloud Collision in Sh2-233 Triggering the Formation of the High-mass Protostar Object IRAS 05358+3543