Empirical velocity profiles for galactic rotation curves
E. Lopez Fune

TL;DR
This paper introduces an empirical model for galaxy rotation curves that fits a large dataset without prior knowledge of luminous matter or fixed dark matter models, revealing a finite galaxy size and enabling total mass estimation.
Contribution
It proposes a unified velocity profile parametrization that accurately fits diverse galaxy rotation curves without pre-assumed luminous or dark matter components.
Findings
Fits 850 galaxy rotation curves accurately
Reveals a finite galaxy size scale
Enables estimation of total galaxy mass
Abstract
A unified parametrization of the circular velocity, which accurately fits 850 galaxy rotation curves without needing in advance the knowledge of the luminous matter components, nor a fixed dark matter halo model, is proposed. A notable feature is that the associated gravitational potential increases with the distance from the galaxy center, giving rise to a length scale indicating a finite size of a galaxy, and after, the Keplerian fall-off of the parametrized circular velocity is recovered according to Newtonian gravity, making possible the estimation of the total mass enclosed by the galaxy.
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