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pro vyhledávání: '"Cha, Heechan"'
We present Spitzer, WISE, and Herschel observations of the young supernova remnant (SNR) N132D in the LMC, including 3-40 microns Spitzer IRS mapping, 12 microns WISE and 70, 100, 160, 250, 350, and 500 microns Herschel images. The high-velocity line
Externí odkaz:
http://arxiv.org/abs/2303.04966
