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A Study of Dark Matter with Spiral Galaxy Rotation Curves. Part II
Universidad San Francisco de Quito, Quito, Ecuador
- 1 Universidad San Francisco de Quito, Quito, Ecuador
International Journal of Astronomy and Astrophysics·Volume 09 (2019)·Pages 133–141·Published 30 April 2019·DOI10.4236/ijaa.2019.92010
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Abstract
In Part II of this study of spiral galaxy rotation curves we apply corrections and estimate all identified systematic uncertainties. We arrive at a detailed, precise, and self-consistent picture of dark matter.
KeywordsDark MatterSpiral GalaxiesDisk GalaxiesMajorana Neutrinos
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