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Fig. 7
Mass flow (Ṁp = 2πsvpΓpρp) along a streamline in the shocked pulsar wind for βp = 0.01 (dotted line), 0.5 (dashed line), and 0.99 (solid line). The mass flow is normalized to the initial mass loss rate of the pulsar, we use ηrel = 1. The simulations with βp = 0.01 and 0.5 give the same results.
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