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Fig. 20

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Number of flow lines that cross the sphere at 4000 AU from the star vs astrospheric longitude. Two cases are illustrated: B = 7 µG (upper panel, model 7) and B = 3 µG (lower panel, model 2). The values of V (2 km s−1) and nH,IS (0.001 cm−3) are the same for both cases.

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