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Fig. 7

image

Value B2 (Eq. (26)) as a function of NFW gravitational potential for each cluster (thin lines). We overplot a thin blue line that shows μ(Φ/Φ0) for Φ0 = −1 700 0002 m2 s-2. Note all clusters lie fairly close to this line, with some discrepancy due to our adopted NFW profile not representing the total potential. This B2 correction to MOND allows the MOND interpolation function to run with the potential as well as the acceleration.

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