Fig. 2.
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Top row: PHANTOM hydrodynamical models of L1551 IRS 5, gas surface density (left) and 100 μm dust particles surface density (right). Bottom row: MCFOST synthetic observations, C18O moment 1 map (left) and continuum emission (right). Snapshots after 13 100 years, which correspond to more than 50 binary orbits. All the images are shown using the same scale (top in au and bottom in arcsec).
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