Reaching the boundary between stellar kinematic groups and very wide binaries - IV. The widest Washington Double Star systems with ρ ≥ 1000 arcsec in Gaia DR3

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Fig. 7

Spatial distribution of the septuple system WDS 19507–5912. The size of the spheres representing every star, labelled in blue, are proportional to their brightness. The projected physical separations from the primary star, HD 188162, in red, are in 10³ au. The overall proper motion, in green, is in mas a⁻¹.

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