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2020ApJ...902...53S - Astrophys. J., 902, 53-53 (2020/October-2)
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.
SANO H., PLUCINSKY P.P., BAMBA A., SHARDA P., FILIPOVIC M.D., LAW C.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. and FUKUI Y.
Abstract (from CDS):
Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.
Journal keyword(s): Supernova remnants - Interstellar medium - Cosmic ray sources - Gamma-ray sources - X-ray sources - Large Magellanic Cloud
Nomenclature: Fig. 5, Table 2: [SPB2020] Cloud A (Nos A-I).
Simbad objects: 39
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