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Fig. 3.
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Same as Fig. 2 but for the low mass outflow rate scenario (Case B, Ṁp = 0.29 M⊙ yr−1). We find that this configuration can predict high polarization values (up to P ≈ 8.8%). The absolute value of polarization reaches its maximum for closer to polar viewing angles (0.4 ≤ |cosΘ|≤0.7 or 45° ≤Θ ≤ 66° & 114° ≤Θ ≤ 135°).
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