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

Abstract

We have carried out a new kinematical analysis of the molecular gas in the Sh2-233 region by using the CO = 2-1 data taken at ∼0.5 pc resolution. The molecular gas consists of a filamentary cloud of 5-pc length with 1.5-pc width where two dense cloud cores are embedded. The filament lies between two clouds, which have a velocity difference of 2.6 km s −1 and are extended over ∼5 pc. We frame a scenario that the two clouds are colliding with each other and compressed the gas between them to form the filament in ∼0.5 Myr which is perpendicular to the collision. It is likely that the collision formed not only the filamentary cloud but also the two dense cores. One of the dense cores is associated with the high-mass protostellar candidate IRAS 05358+3543, a representative high-mass protostar. In the monolithic collapse scheme of high mass star formation, a compact dense core of 100 ⊙ 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 previous works. We argue that the proposed collision is a step which efficiently collects the gas of 100 ⊙ into 0.1 pc radius. This lends support for that the cloud-cloud collision is an essential process in forming the compact high-mass dense core, IRAS 05358+3543.

Modelo computacional de la formación de cúmulos proto-estelares

“…Cabe aclarar que, sin esta velocidad traslacional, las sub-nubes no colisionarían, pues como mostramos en la Figura 3, una nube turbulenta terminaría con un colapso anisotrópico central. Por otro lado, existe amplia evidencia observacional de la ocurrencia de colisiones entre nubes moleculares [5]. Una posible explicación de la ocurrencia de colisiones entre nubes-que se mueven principalmente siguiendo la rotación de la Galaxia-es que se han observado nubes que también se mueven en direcciones aleatorias en el plano de la Galaxia [6] y [7].…”

Simulations of Unequal Binary Collisions Embedded in a Turbulent Gas Cloud Far From a Massive Gravitational Center

“…There is ample observational evidence of the occurrence of cloud-cloud collisions, see Testi et al (2000), Churchwell et al (2006), Furukawa et al (2009), Torii et al (2011), Takahira et al (2014) and Yamada et al (2021). Regions such as RCW49, Westerlund2, and NGC 3603 are examples of cloudcloud collisions.…”