Fig. 10
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Evolution of the bright bow shock in the C1h and C1k regions. The top, middle and bottom panels show the same area of the sky at the three different epochs (2003, 2012, and 2020). The fast moving flow (υtg ~ 100–120 km s−1) corresponding to B3 shocks against the C1h and C1k regions (υtg ~ 10–70 km s−1) producing a bright bow shock. The PMs of knots are shown as in Fig. 8.
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