Figure 4 from Confronting the Jet Model of Sgr A* with the Faraday Rotation Measure Observations

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Confronting the Jet Model of Sgr A* with the Faraday Rotation Measure Observations

Authors: Ya-Ping Li, Feng Yuan, and Q. Daniel Wang

Li, Yuan, & Wang 2015 The Astrophysical Journal 798 22.

Provider: AAS Journals

Caption: Figure 4.

RM contribution from the accretion flow as a function of the viewing angle for four different model parameter sets (p, β). Only the red solid and blue dotted lines, which correspond to p = 1.0 and β = 0.5–0.9, can reach the magnitude of the observed RM, ~10⁵ rad m⁻².

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