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Relativistic X-Ray Reverberation from Super-Eddington Accretion Flow

  • Authors: Lars Lund Thomsen, Lixin Dai, Erin Kara, and Chris Reynolds

2022 The Astrophysical Journal 925 151.

  • Provider: AAS Journals

Caption: Figure 6.

Lag–frequency spectra: the frequency and time units are expressed in natural units. The BH spin a = 0.8, and the reflection surface is cut at Rout = 1000 Rg in all cases. The shaded region is the low-frequency band used to calculate the energy-dependent lags in Section 3.2.2. (a) Comparison between the SE and thin disk cases (see labels for the configurations). hLP is fixed at 10Rg. (b) Comparison between different hLP for the SE disk.

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