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We present the results of a study of the spatial distribution relative to bright normal galaxies of a new large sample of blue compact galaxies (BCGs) in the zone of the Second Byurakan Survey (SBS): 7ʰ⁴0ᵐ^ 5 h^-1^ Mpc and are found in voids. The large deficiency of BCGs with DNN_ <~ 2 h¹^ Mpc supports the hypothesis that the majority of dwarf galaxies originate as low-mass primordial density fluctuations, but not as debris resulting from tidal interactions between massive galaxies. The spatial distribution of BCGs is consistent with that found for low-surface- brightness dwarfs, supporting the idea that BCGs are LSB dwarfs undergoing intense bursts of star formation.
Pustilnik et al. (Sat,) studied this question.