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X-RAY FADING AND EXPANSION IN THE “MINIATURE SUPERNOVA REMNANT” OF GK PERSEI

  • Authors: D. Takei, J. J. Drake, H. Yamaguchi, P. Slane, Y. Uchiyama, and S. Katsuda

2015 The Astrophysical Journal 801 92.

  • Provider: AAS Journals

Caption: Figure 4.

Comparison of background-subtracted SB radial profiles of GK Per in 2000 (black) and 2013 (red) in the 0.5–1.2 keV band computed from the exposure-corrected photon-flux images, taking into account the degradation of the quantum efficiency of ACIS-S3. The dashed lines show 0.6 keV PSFs that were normalized to the maxima of the observed peaks, and further to the minima of the background levels. The lower panel indicates the ratios of 2013 to 2000 data, suggesting that the SB drop was 36% ± 6% in the 20″–40″ plateau area, which is indicated by the orange region and the dashed–dotted lines.

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