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 Journal14899.
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.