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Retarded Evolution of Low-Mass Galaxies in Voids?
2006
Proceedings of the International Astronomical Union
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We analyze possible differences in the global environments of very metal-poor BCGs with that of typical metallicity BCGs, basing on the parameter DNN -distance to the nearest "luminous" galaxy. We find very significant difference suggesting that a higher fraction of unevolved dwarfs reside in 'voids'.
doi:10.1017/s1743921306006417
fatcat:zubxhguakje27gmajwqidj6g5m