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Fig. 3
Evolution of the Stokes function at the crust of the LM model. Each panel corresponds to a different accretion rate. In both panels, each curve (from top to bottom at the NS surface RNS) corresponds to t = 1, 101, 102, 103, 104, 105, 106, and 107 yr. In all cases, we use Q = 5 and no SF model.
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