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- W1816650832 abstract "The rotation curves of disk galaxies exhibit a number of striking regularities. The amplitude of the rotation is correlated with luminosity (Tully-Fisher), the shape of the rotation curve is well predicted by the luminous mass distribution, and the magnitude of the mass discrepancy increases systematically with decreasing centripetal acceleration. These properties indicate a tight connection between light and mass, and impose strong constraints on theories of galaxy formation." @default.
- W1816650832 created "2016-06-24" @default.
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- W1816650832 date "1999-09-27" @default.
- W1816650832 modified "2023-09-27" @default.
- W1816650832 title "Dynamical Constraints on Disk Galaxy Formation" @default.
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