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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 10.

Distribution of spectral peaks (top panel) and spectral peak widths (bottom panel) for ﹩\beta =0.125﹩ (solid lines), ﹩\beta =1﹩ (dashed lines), and ﹩\beta =2﹩ (dotted lines) for ﹩a=0.5﹩, ﹩i=82\buildrel{\circ}\over{.} 5﹩.

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