FOREST unbiased Galactic plane imaging survey with the Nobeyama 45 m telescope (FUGIN). VI. Dense gas and mini-starbursts in the W 43 giant molecular cloud complex
Abstract
We performed new large-scale 12CO, 13CO, and C18O J = 1-0 observations of the W 43 giant molecular cloud complex in the tangential direction of the Scutum arm (l ∼30°) as a part of the FUGIN project. The low-density gas traced by 12CO is distributed over 150 pc × 100 pc (l × b), and has a large velocity dispersion (20-30 km s-1). However, the dense gas traced by C18O is localized in the W 43 Main, G30.5, and W 43 South (G29.96-0.02) high-mass star-forming regions in the W 43 giant molecular cloud (GMC) complex, which have clumpy structures. We found at least two clouds with a velocity difference of ∼10-20 km s-1, both of which are likely to be physically associated with these high-mass star-forming regions based on the results of high 13CO J = 3-2 to J = 1-0 intensity ratio and morphological correspondence with the infrared dust emission. The velocity separation of these clouds in W 43 Main, G30.5, and W 43 South is too large for each cloud to be gravitationally bound. We also revealed that the dense gas in the W 43 GMC has a high local column density, while "the current SFE" (star formation efficiency) of the entire GMC is low ( $\sim\!\! 4\%$ ) compared with the W 51 and M 17 GMC. We argue that the supersonic cloud-cloud collision hypothesis can explain the origin of the local mini-starbursts and dense gas formation in the W 43 GMC complex.
- Publication:
-
Publications of the Astronomical Society of Japan
- Pub Date:
- January 2021
- DOI:
- 10.1093/pasj/psaa015
- arXiv:
- arXiv:2001.10693
- Bibcode:
- 2021PASJ...73S.129K
- Keywords:
-
- HII regions;
- ISM: clouds;
- ISM: molecules;
- stars: formation;
- ISM: individual objects (W 43;
- W 43 Main;
- G30.5;
- W 43 South;
- G29.96-0.02);
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 51 pages, 34 figures, 6 tables, accepted for publication in PASJ