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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 3.

Radial projection profiles in the 0.5–1.2 keV band derived from the rectangular regions in Figure 1, smoothed by Gaussian blurs of 5 pixel radius at 2σ, are shown color-coded (black for 2000 and red for 2013). The vertical dotted lines mark the positions of the peak of the rim emission and the dashed–dotted lines are the half-maximum levels of each profile. Both indicate that the observed expansion of the X-ray nebula is approximately 1″–2″ in 13.8 yr. The typical 1σ uncertainties of the data points are represented by the vertical bars.

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