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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 ProtonsDOI: info:10.3847/1538-4357/abb469v. 90253
Sano, H., Plucinsky, Paul P., Bamba, A., Sharda, P., Filipovic, M. D., Law, Charles J., Alsaberi, R. Z. E., Yamane, Y., Tokuda, K., Acero, F., Sasaki, M., Vink, J., Inoue, T., Inutsuka, S., Shimoda, J., Tsuge, K., Fujii, K., Voisin, F., Maxted, N., Rowell, G., Onishi, T., Kawamura, A., Mizuno, N., Yamamoto, H., Tachihara, K. et al. 2020. "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." The Astrophysical Journal, 902 53. https://doi.org/10.3847/1538-4357/abb469.
Spatially Resolved Chandra Spectroscopy of the Large Magellanic Cloud Supernova Remnant N132DDOI: info:10.3847/1538-4357/ab8a46v. 894145
Sharda, Piyush, Gaetz, Terrance J., Kashyap, Vinay L., and Plucinsky, Paul P. 2020. "Spatially Resolved Chandra Spectroscopy of the Large Magellanic Cloud Supernova Remnant N132D." The Astrophysical Journal, 894 145. https://doi.org/10.3847/1538-4357/ab8a46.