Variable Modified Newtonian Mechanics VIII: Ultra faint dwarfs in Milky Way
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.
Fields of Study & Subjects
Galaxies: Formation
Evolution
Phenomena
Cosmology and Gravitation Theories
Stellar
planetary
and galactic studies
Publication details
- Journal / source
- arXiv (Cornell University)
- Publication date
- 4 February 2026
- Document type
- Preprint