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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 1.

A picture of our ADAF-jet model, where a geometrical thick, optically thin ADAF and parabolic shape of jet are considered. The jet inclination angle is assumed to be 15o, and the disk is perpendicular to the jet. Here, we consider the two possibilities where the polarized emission passes through ADAF itself along LOS-1 and the polarized emission of ADAF passes through the plasma in the jet along LOS-2 (the thick solid lines).

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