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Fig. 21
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Longitude-latitude distribution of the flow lines crossing points on a sphere with a radius of 4000 AU and the centre at the host star for the case V = 2 km s−1, B = 7 µG, nH,IS = 0.001 cm−3 (model 7). In addition to the R and L streams, there are a few crossing points in the tail region (less than 1% of the total flux).
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