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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 2.

Hα map of the LMC (Image Credit: C. Smith, S. Points, the MCELS Team and NOAO/AURA/NSF). The 16 LMC SNRs used in this study are marked with circles. A larger circle implies a brighter SNR in a square-root scale. Blue circles indicate that the SNR is located within a star-formation region, while red circles indicate that the SNR is not located within a star-formation region. The SNRs used in H98 are underlined.

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