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Modeling the Spectral Signatures of Accretion Disk Winds: A New Monte Carlo Approach

  • Authors: Knox S. Long and Christian Knigge

Long & Knigge 2002 The Astrophysical Journal 579 725.

  • Provider: AAS Journals

Caption: Fig. 3.

Comparison of ionization fractions of He, C, Ni, and O as calculated using CLOUDY (left) and with the modified on‐the‐spot approximation used within PYTHON (right) for a blackbody radiation field with an effective dilution factor W of 0.01. Neutral species as well as He II, C IV, N V, and O VI appear as black lines in the figure.

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