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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 5.

Comparison of 0.5–1.2 keV background-subtracted azimuthal dependence in integrated flux in 2000 (black) and 2013 (red). The solid and dashed–dotted lines are the results of using different background estimates; the former used the one-eighth outward sectors at each azimuth angle, of which the background levels are shown by the dashed lines, while the latter is from the entire background annulus (see Figure 1 for details). The 1σ confidence ranges of the former estimates are illustrated by the color-coded bands. The lower panel indicates the ratios of 2013 to 2000 data.

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