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A Multiscale Molecular and Atomic Gas View on the H II Region N113 in the Large Magellanic Cloud: Evidence for High-mass Star Formation Triggered by Supersonically Colliding H I Flows

  • Authors: Rin I. Yamada, Kazuki Tokuda, Yasuo Fukui, Daiki Adachi, Marta Sewiło, Rémy Indebetouw, C.-H. Rosie Chen, Kisetsu Tsuge, Takeru Nishioka, Hidetoshi Sano, Mao Tamashiro, Naslim Neelamkodan, Tony Wong, Lynn R. Carlson, Joana M. Oliveira, Akiko Kawamura, Kengo Tachihara, Toshikazu Onishi

Rin I. Yamada et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure B2.

Normalized spectrum of N113 GMC in 12CO(J = 2–1) and 12CO(J = 1–0) obtained with APEX and MOPRA, respectively. For the APEX data, we derived the average spectrum over the entire observed field. For the MOPRA data, only the area overlapping the APEX coverage was extracted, and the average spectrum within this region was obtained. Both spectra were normalized such that their peak intensities are unity. The red and blue transparent belts indicate the velocity range of the D-component and L-component, respectively. The two CO emission lines are located in the velocity range of the D-component.

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