Fig. 5.

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Same as Fig. 4 but for Case B, Ṁp = 0.29 M⊙ yr−1, and for simulations: s3) Rph = 1014 cm, Rint = 5 × 1014 cm, Δθ = 45° (left column and top panel of middle column) and s4) Rph = 1014 cm, Rint = 5 × 1014 cm, Δθ = 180° (right column and bottom panel of middle column). The gray dashed line circle here denotes the projection for each observer of the electron scattering photosphere with radius dsc_ph.
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