Galactic Magnetic Fields. I. Theoretical Model and Scaling Relations
Galactic dynamo models have generally relied on input parameters that are very challenging to constrain. We address this problem by developing a model that uses observable quantities as input: the galaxy rotation curve, the surface densities of the gas ...
Luke Chamandy +2 more
doaj +1 more source
Can rotation curves reveal the opacity of spiral galaxies? [PDF]
A. Misiriotis
openalex +1 more source
Galaxy rotation curves using a non-parametric regression method: core, cuspy and fuzzy scalar field dark matter models [PDF]
Lizbeth M. Fernández-Hernández +2 more
openalex +1 more source
Gravito-Electrodynamics in Galaxy Rotation Curves. ENG: An Extended Newtonian Gravitation
Barbaro Quintero-Leyva
openalex +2 more sources
Discs no more: the morphology of low-mass simulated galaxies in FIREbox. [PDF]
Benavides JA +11 more
europepmc +1 more source
Prediction Note: Geometry-Dependent Residual Structure in Galaxy Rotation Curves
Wilhoite, Sean
openalex +1 more source
A giant disk galaxy two billion years after the Big Bang. [PDF]
Wang W +16 more
europepmc +1 more source
An explanation for galaxy rotation curves using a Clifford multivector spacetime framework [PDF]
James M. Chappell +3 more
openalex +1 more source
Milky Way could invalidate the hypothesis of exotic matter and favor a gravitomagnetic solution to explain dark matter. [PDF]
Le Corre S.
europepmc +1 more source

