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 Journal151161.
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.