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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 4.

Spectral model fits for three representative regions in DEM L71. In all fits, metal abundances are fixed at our measured LMC abundance values (Table 2). ISM-only (yellow region), metal-rich ejecta only (red region), and their combined spectra. The residuals from the spectral model fits are shown at the bottom panel of each spectral plot. Green regions are the other regions used in our ISM abundance measurements.

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