Modified gravity (MOG) and the cluster Abell 1689 acceleration data
  The galaxy cluster system Abell 1689 has been well studied and yields good
lensing and X-ray gas data. Modified gravity (MOG) is applied to the cluster
Abell 1689 and the acceleration data is well fitted without assuming dark
matter. Newtonian dynamics and Modified Newtonian dynamics (MOND) are shown not
to fit the acceleration data, while a dark matter model based on the
Navarro-Frenk-White (NFW) mass profile is shown to fit the acceleration data
for the radial range $r > 200$ kpc.
