Fig. 15
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Mid-plane density ρmax, aspect ratio H(r)/r, and density scale height H(r) (Eq. (7)), for model v05e00, at four different θ quadrants centred around θ = 0, π/2, π and 3π/2, and averaged over all θ (full, black line), giving insight into the asymmetric nature of the accretion disk. θ = 0 is the side away from AGB star, as shown in Fig. C.6.
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