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HFPK 334: An Unusual Supernova Remnant in the Small Magellanic Cloud
Crawford et al. 2014 The Astronomical Journal 148 99.
Caption: Figure 6.
Co-fit Chandra (point source: red; diffuse emission: green) and XMM-Newton (black) spectra with the best-fit model overlaid.
© 2014. The American Astronomical Society. All rights reserved.