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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 7.

﹩{\chi }_{\nu }^{2}﹩ maps of N63A based on our spectral model fits for 346 adaptive mesh-created regions (see Section 4.2). (A) The ﹩{\chi }_{\nu }^{2}﹩ map for spectral model fits with abundances fixed at the mean ISM values of this work. (B) The ﹩{\chi }_{\nu }^{2}﹩ map for spectral model fits with abundances fixed at the mean ISM values from H98.

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