Fig. 4.
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Proper motions (velocity projected in the plane of the sky) of the known TTSs in the TAMC with high-quality astrometric measurements (RUWE < 1.4). CTTSs and WTTSs are represented with blue and red arrows, respectively. We note that the motion of the stars is not parallel to the filaments and is approximately perpendicular to the direction of the magnetic field.
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