Radial Acceleration Relation in Rotationally Supported Galaxies.

  title={Radial Acceleration Relation in Rotationally Supported Galaxies.},
  author={Stacy S. McGaugh and Federico Lelli and James M. Schombert},
  journal={Physical review letters},
  volume={117 20},
We report a correlation between the radial acceleration traced by rotation curves and that predicted by the observed distribution of baryons. The same relation is followed by 2693 points in 153 galaxies with very different morphologies, masses, sizes, and gas fractions. The correlation persists even when dark matter dominates. Consequently, the dark matter contribution is fully specified by that of the baryons. The observed scatter is small and largely dominated by observational uncertainties… Expand

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