Variable Modified Newtonian Mechanics VIII: Ultra faint dwarfs in Milky Way
arXiv:2602.04273
Abstract
Velocity dispersions of Ultra faint dwarf (UFD) galaxies are observed to deviate significantly from the Baryon Tully Fisher Relation of the massive galaxies (BTFR). We propose a solution with Variable Modified Newtonian dynamics model, which could explain this deviation.
23 pages 0 figures