Abell 1758N from an optical point of view: new insights on a merging cluster with diffuse radio emission

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Fig. 12

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Dendogram obtained through the Serna & Gerbal (1996) algorithm. The abscissa is the binding energy (here in arbitrary units with the deepest negative energy levels on the left) while the catalog numbers of the various member galaxies are shown along the ordinate (IDm in Table 1).

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