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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 3.

Four snapshots of a caustic with caustic crossing angle ﹩{\theta }_{{\rm{c}}}=90^\circ ﹩ moving from the right to the left. The left panels show the magnification-weighted surface brightness with a logarithmic color scale. The right panels show the corresponding energy spectra of the Fe Kα emission. All panels: ﹩a=0.5﹩, ﹩i=82\mathop{.}\limits^{^\circ }5﹩, ﹩\beta =0.5﹩.

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