Figure 3 from AN ACCRETION-JET MODEL FOR M87: INTERPRETING THE SPECTRAL ENERGY DISTRIBUTION AND FARADAY ROTATION MEASURE

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AN ACCRETION-JET MODEL FOR M87: INTERPRETING THE SPECTRAL ENERGY DISTRIBUTION AND FARADAY ROTATION MEASURE

Authors: Jianchao Feng, Qingwen Wu, and Ru-Sen Lu

2016 The Astrophysical Journal 830 6.

Provider: AAS Journals

Caption: Figure 3.

Intensity distribution at 230 GHz from the ADAF (top panel) and jet (bottom panel) models, where the model parameters are the same as those adopted in the SED modeling in Figure 2.

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