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• W4205220304 abstract "The dynamics of isolated galaxy pairs represents an important tool to investigate the behavior of gravity in the low acceleration regime. Statistical analysis of a large sample of galaxy pairs led to the noticeable discovery of a region of preferred 3-dimensional velocities centered at $sim 150$ km/s and $sim 100$ km/s wide, a feature hard to justify in the context of numerical simulations of cosmological structure formation. It is shown here that such a feature is expected within the framework of the Modified Newtonian Dynamics, which, however, predicts it to be centered at $sim$ 170 Km/s." @default.
• W4205220304 created "2022-01-25" @default.
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• W4205220304 date "2021-12-16" @default.
• W4205220304 modified "2023-09-24" @default.
• W4205220304 title "On the orbital velocity of isolated galaxy pairs: a test of gravity in the low acceleration regime" @default.
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• W4205220304 doi "https://doi.org/10.1093/mnras/stab3636" @default.
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