Molecular gas in a Spitzer bubble N4: possible evidence for cloud-cloud collisions as a trigger of massive star formation
Shinji Fujita, Kazufumi Torii, Kengo Tachihara, Rei Enokiya, Katsuhiro, Hayashi, Nario Kuno, Mikito Kohno, Tomoka Tosaki, Mitsuyoshi Yamagishi,, Atsushi Nishimura, Tomofumi Umemoto, Tetsuhiro Minamidani, Mitsuhiro Matsuo,, Yuya Tsuda, Hidetoshi Sano, Daichi Tsutsumi, Akio Ohama

TL;DR
This study presents CO emission observations of the Spitzer bubble N4, providing evidence that cloud-cloud collisions may have triggered massive star formation in this region.
Contribution
It offers new observational evidence of cloud-cloud collisions in N4, linking these interactions to the initiation of massive star formation.
Findings
Identification of three discrete velocity clouds in N4.
Detection of bridge features and complementary distribution indicating cloud collisions.
Evidence of star formation triggered by cloud collisions in N4 and N4W.
Abstract
Herein, we present the 12CO (J=1-0) and 13CO (J=1-0) emission line observations via the FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) toward a Spitzer bubble N4. We observed clouds of three discrete velocities: 16, 19, and 25 km/s. Their masses were 0.1x10^4 Msun, 0.3x10^4 Msun, and 1.4x10^4 Msun, respectively. The distribution of the 25-km/s cloud likely traces the ring-like structure observed at mid-infrared wavelength. We could not find clear expanding motion of the molecular gas in N4. On the contrary, we found a bridge feature and a complementary distribution, which are discussed as observational signatures of a cloud-cloud collision, between the 16- and 25-km/s clouds. We proposed a possible scenario wherein the formation of a massive star in N4 was triggered by a collision between the two clouds; however whereas the 19-km/s cloud is…
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