Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 2.

The 12CO(J = 2–1) (upper panel) and 13CO(J = 2–1) (lower panel) integrated intensity (moment 0; (a) and (d)), mean velocity (moment 1; (b) and (c)), and velocity dispersion (moment 2; (c) and (f)) images of N113. The white crosses represent the positions of YSOs and YSO candidates (B. A. Whitney et al. 2008; R. A. Gruendl & Y.-H. Chu 2009; J. P. Seale et al. 2009; L. R. Carlson et al. 2012). The beam size is shown in the lower left corner of each image.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse