FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45 m telescope (FUGIN): Molecular clouds toward W 33; possible evidence for a cloud-cloud collision triggering O star formation

We observed molecular clouds in the W 33 high-mass star-forming region associated with compact and extended H 11 regions using the NANTEN2 telescope as well as the Nobeyama 45 m telescope in the J = 1-0 transitions of (CO)-C-12, (CO)-C-13, and (CO)-O-18 as part of the FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45 m telescope (FUGIN) legacy survey. We detected three velocity components at 35 km s(-1), 45 km s(-1), and 58 km s(-1). The 35 km s(-1) and 58 km s(-1) clouds are likely to be physically associated with W 33 because of the enhanced (CO)-C-12 J = 3-2 to J = 1-0 intensity ratio as R3-2/1-0 > 1.0 due to the ultraviolet irradiation by OB stars, and morphological correspondence between the distributions of molecular gas and the infrared and radio continuum emissions excited by high-mass stars. The two clouds show complementary distributions around W 33. The velocity separation is too large to be gravitationally bound, and yet not explained by expanding motion by stellar feedback. Therefore, we discuss whether a cloud-cloud collision scenario likely explains the high-mass star formation in W 33.