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Synthetic rotation curves of spiral galaxies

1997
We 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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Dark Matter Particles and the Flat Rotation Curves of Spiral Galaxies

Astrophysics and Space Science, 1995
Heinz Dehnen
exaly  

Rotation Curves of Galaxies in Various Space Environments

Astrophysics, 2001
Vladimir Reshetnikov, E A Evstigneeva
exaly  

The Carmeli Metric Correctly Describes Spiral Galaxy Rotation Curves

International Journal of Theoretical Physics, 2005
exaly  

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