Modeling of interactions between supernovae ejecta and aspherical circumstellar environments

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Fig. 7

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Model A: as in Fig. 6, with the slope parameters n = 9 and w_sw = 2, in the polar direction (the same method of calculation as in Fig. 6). The semi-analytical profiles are compared to the same polar expansion velocity as in Figs. 4 and 6.

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