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Fig. 2.
Proper motion distribution for stars in a region of radius 80 arcmin around the nominal centre of Rup 147, coloured according to parallax (Gaia Collaboration 2018b). Candidate member stars in Rup 147 show a well clustered distribution roughly centred on PMα, PMδ ≈ −1, −26 and ϖ ≈ 3.
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