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Fig. 5.

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Dependence of the Hubble flow fit on the minimum distance from the barycentre for the minor (left column) and major infall models (right column). The first and third rows have M 81 as the centre of mass. The second and fourth row use the barycentre located on the connection line between M 81 and M 82. The first and second row use vhel. The third and fourth row use vLG. For the major infall model, velocities up to a maximum value of 700 km/s were included in the fit.

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