Molecular clouds in the NGC 6334 and NGC 6357 region: Evidence for a 100 pc-scale cloud–cloud collision triggering the Galactic mini-starbursts. (30th March 2018)

• Record Type: Journal Article
• Authors: Fukui, Yasuo; Kohno, Mikito; Yokoyama, Keiko; Torii, Kazufumi; Hattori, Yusuke; Sano, Hidetoshi; Nishimura, Atsushi; Ohama, Akio; Yamamoto, Hiroaki; Tachihara, Kengo
• Is Part Of: Publications of the Astronomical Society of Japan. Volume 70:Number SP2(2018)
• Publication Date: 2018-03-30
• Subjects: ISM: clouds -- ISM: individual objects (NGC 6334, NGC 6357) -- stars: formation; Astronomy -- Periodicals; 520.5
• DOI: 10.1093/pasj/psy017
• Languages: English
• ISSNs: 0004-6264

Abstract

Abstract: We carried out new CO ( J = 1–0, 2–1, and 3–2) observations with NANTEN2 and ASTE in the region of the twin Galactic mini-starbursts NGC 6334 and NGC 6357. We detected two velocity molecular components of 12 km s −1 velocity separation, which is continuous over 3° along the plane. In NGC 6334 the two components show similar two-peaked intensity distributions toward the young H ii regions and are linked by a bridge feature. In NGC 6357 we found spatially complementary distribution between the two velocity components as well as a bridge feature in velocity. Based on these results we hypothesize that the two clouds in the two regions collided with each other in the past few Myr and triggered the formation of the starbursts over ∼ 100 pc. We suggest that the formation of the starbursts happened toward the collisional region of extent ∼ 10 pc with initial high molecular column densities. For NGC 6334 we present a scenario which includes spatial variation of the colliding epoch due to non-uniform cloud separation. The scenario possibly explains the apparent age differences among the young O stars in NGC 6334, which range from 10 4 yr to 10 6 yr; the latest collision happened within 10 5 yr toward the youngest stars in NGC 6334 I(N) and I which exhibit molecular outflows without H ii regions. For NGC 6357 the O stars were formed a few Myr ago, and the cloud dispersal by the O stars is significant. We conclude that cloud–cloud collision offers a possible explanation of the mini-starburst over a 100 pc scale.