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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 6.

(a) Integrated intensity map of H I clouds around N113 (image: D-component, contours: L-component). The green dashed square indicates the ALMA+APEX FoV. (b) H I position–velocity cut along “slice 1” indicated in (a). The diagram is along the OFFSET-X and OFFSET-Y coordinates, which are rotated 15° clockwise from the J2000 coordinate, with the rotation origin being the center of the ALMA+APEX FoV. Contours are plotted every 10 K starting at 5 K. (c) Same as (b), but for slice 2 in (a). The white cross indicates an approximate spatial and spectral extent of the CO emission in N113. The black dashed lines in the figure indicate the approximate offset-X positions where the I-component is clearly seen as a bridge connecting the L-component and the D-component.

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