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Fig. 5.
Distribution of the most luminous dSph satellites of the Milky Way (Fornax, Leo I, Sculptor, and Leo II), M 31 (NGC 147, And II, And I, CasSph, and PegSph), M 81 (KDG61, KDG64, KDG63, and F8D1), and NGC 253 (SC 22) according to their integrated absolute B-magnitude and the linear Holmberg’s diameter A26.
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