A simple model for explaining Galaxy Rotation Curves
arXiv:1804.09620 · doi:10.3390/galaxies6030070
Abstract
A new simple expression for the circular velocity of spiral galaxies is proposed and tested against HI Nearby Galaxy Survey (THINGS) data set. Its accuracy is compared with the one coming from MOND.
arXiv comment9 pages, 3 figures, 2 tables; this article is connected to arXiv:1705.04131
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