Paper:	Revealing the Large-Scale Structures of Interstellar Gas Associated with the Magellanic SNR N132D
Volume:	499, Revolution in Astronomy with ALMA: The Third Year
Page:	257
Authors:	Sano, H.; Fukui, Y.; Yoshiike, S.; Fukuda, T.; Tachihara, K.; Inutsuka, S.; Kawamura, A.; Fujii, K.; Mizuno, N.; Inoue, T.; Onishi, T.; Acero, F.; Vink, J.
Abstract:	We report preliminary results of large-scale distribution toward the Magellanic supernova remnant N132D using Mopra and Chandra archival datasets. We identified a cavity-like CO structure along the X-ray shell toward the southern half of it. The total mass of associating molecular gas is ∼104 M☉, which is smaller than the previous study by an order of magnitude. Further observations using ALMA, ASTE, and Mopra will reveal the detailed spatial structures and its physical conditions.

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