Image Details
Caption: Figure 12.
A selection of polarimetric observables plotted as a function of inclination in a slice of our parameter space corresponding to MAD a * = 0.94, R high = 10 reversed models. In very ordered models such as this one, symmetry and cancellation lead to the smallest net linear polarization fractions for face-on viewing angles at the same time that the resolved linear polarization fraction is highest. In this model, ∠β 2 encodes the direction of motion, and v net encodes the direction of the magnetic field with respect to the line of sight.
© 2024. The Author(s). Published by the American Astronomical Society.