Figure 1 from A CHANDRA STUDY OF THE INTERSTELLAR METALLICITY IN THE LARGE MAGELLANIC CLOUD USING SUPERNOVA REMNANTS

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A CHANDRA STUDY OF THE INTERSTELLAR METALLICITY IN THE LARGE MAGELLANIC CLOUD USING SUPERNOVA REMNANTS

Authors: Andrew Schenck, Sangwook Park, and Seth Post

2016 The Astronomical Journal 151 161.

Provider: AAS Journals

Caption: Figure 1.

Three-color maps for individual SNRs with ISM regions used for spectral modeling overlaid. Color codes are red: 300–720 eV, green: 720–1100 eV, blue: 1100–7000 eV. 0519-69.0 and N206 have been adaptively smoothed to emphasize their faint ISM features.

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