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Cited article:

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Astronomy & Astrophysics 687 A26 (2024)
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High-mass star formation in the Large Magellanic Cloud triggered by colliding H i flows

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Publications of the Astronomical Society of Japan 76 (4) 589 (2024)
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Three-dimensional geometry and dust/gas ratios in massive star-forming regions over the entire LMC as revealed by the IRSF/SIRIUS survey

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Publications of the Astronomical Society of Japan 74 (3) 639 (2022)
https://doi.org/10.1093/pasj/psac025

ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons

H. Sano, P. P. Plucinsky, A. Bamba, P. Sharda, M. D. Filipović, C. J. Law, R. Z. E. Alsaberi, Y. Yamane, K. Tokuda, F. Acero, M. Sasaki, J. Vink, T. Inoue, S. Inutsuka, J. Shimoda, K. Tsuge, K. Fujii, F. Voisin, N. Maxted, G. Rowell, T. Onishi, A. Kawamura, N. Mizuno, H. Yamamoto, K. Tachihara and Y. Fukui
The Astrophysical Journal 902 (1) 53 (2020)
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Using CO line ratios to trace compressed areas in bubble N131

Chuan-Peng Zhang, Guang-Xing Li, Chenlin Zhou, Lixia Yuan and Ming Zhu
Astronomy & Astrophysics 631 A110 (2019)
https://doi.org/10.1051/0004-6361/201936063