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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)
DOI: 10.3847/1538-4357/abb469
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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)
DOI: 10.1051/0004-6361/201936063
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