Wielkoskalowa struktura Wszechświata 2007

Wielkoskalowa struktura Wszechświata 2007 Wielkoskalowa struktura Wszechświata 2007

11.07.2015 Views

A linear galaxy vs DM bias, at 8 Mpc scale, seemsto evolve faster for galaxies brighter than M*

Does a galaxy bias (computed at the 8 Mpc scale)vs DM change with redshift differently for galaxieswith different stellar masses?

A linear galaxy vs DM bias, at 8 Mpc scale, seemsto evolve faster for galaxies brighter than M*

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