Figure 6 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 6.

Averaged elemental abundances estimated by our plane-shock model fits to integrated ACIS and ASCA spectra of the seven SNRs used in H98. Elemental abundances from this work and H98 are also shown. Statistical uncertainties have a 90% confidence level.

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