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grmonty: A Monte Carlo Code for Relativistic Radiative Transport

  • Authors: Joshua C. Dolence, Charles F. Gammie, Monika Mościbrodzka, and Po Kin Leung

DOLENCE et al. 2009 The Astrophysical Journal Supplement Series 184 387.

  • Provider: AAS Journals

Caption: Figure 7.

Spectra (upper panel) from grmonty (points) and sphere (solid line) produced by Comptonization of soft photons in a homogeneous, spherical cloud of hot plasma. Computations are done for: plasma optical thickness τ = 10 −4, plasma temperature Θ e = 4, and the central source radiative temperature kT r / m ec = 10 −8. Lower panel shows the fractional difference between the two spectra.

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