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HFPK 334: An Unusual Supernova Remnant in the Small Magellanic Cloud

  • Authors: E. J. Crawford, M. D. Filipović, R. L. McEntaffer, T. Brantseg, K. Heitritter, Q. Roper, F. Haberl, and D. Urošević

Crawford et al. 2014 The Astronomical Journal 148 99.

  • Provider: AAS Journals

Caption: Figure 3.

Chandra three color composite (red: 0.3–1.0 keV (soft), green: 1.0–2.0 keV (medium), blue: 2.0–6.0 keV (hard)) smoothed with a Gaussian width to match the 20 cm radio image. The radio contours are 0.6–1.6 mJy beam−1 in 0.2 mJy beam−1 steps.

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