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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 5.

Integrated intensity maps of H I clouds around N113. The velocity range over which the emission was integrated is (−50.1, −30.5) km s−1 for the L-component (panel (a)) and (−10.4, 9.8) km s−1 for the D-component (panel (b)). The green dashed square indicates the ALMA+APEX field of view (FoV). Contours are plotted every 70 from 60 K km s–1 for (a) and 150 K km s−1from 10 K km s−1 for (b).

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