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Simulations of the Fe Kα Energy Spectra from Gravitationally Microlensed Quasars

  • Authors: H. Krawczynski and G. Chartas

2017 The Astrophysical Journal 843 118.

  • Provider: AAS Journals

Caption: Figure 11.

Magnification-weighted surface brightness (logarithmic color scale) for the same configuration as the top panel of Figure 3 but for an increased absorption probability (top panels, ﹩{p}_{\mathrm{abs}}=0.99﹩ instead of ﹩{p}_{\mathrm{abs}}=0.9﹩) and for an increased likelihood of scattering rather than Fe Kα emission (bottom panels, ﹩R=5﹩ rather than ﹩R=1﹩).

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