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Synthetic rotation curves of spiral galaxies
1997We analyse the shape of the rotation curves by means of the Principal Component Analysis (PCA) and find that the first two principal components account for about 90% of the total variance in rotation curve shapes. The most important physical parameter (the first principal component) works for the rotation curve in a similar way at all positions within ...
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On the use of galaxy rotation curves to test the modified dynamics
Astrophysical Journal, 1988Mordehai Milgrom
exaly
Galaxy rotation curves from general relativity with renormalization group corrections
Journal of Cosmology and Astroparticle Physics, 2010Davi C Rodrigues +2 more
exaly

