Results 141 to 150 of about 64,819 (265)
While galaxy rotation curves (RCs) provide one of the most powerful methods for measuring dark matter profiles in the inner regions of rotation-supported galaxies, at the dwarf scale there are factors that can complicate this analysis.
Isabel S. Sands +11 more
doaj +1 more source
Galaxy rotation curves in the $\mu$-deformation based approach. [PDF]
A. M. Gavrilik +2 more
openalex
Modelling the rotational curves of spiral galaxies with a scalar field [PDF]
J. P. Mbelek
openalex +1 more source
Chameleon gravity as an alternative to dark matter
By studying the chameleon gravity on galaxy scales, we investigate the effects of the chameleon dark matter. To perform this task, we consider the dynamics of the chameleon scalar field in the region of galactic halos in static spherically symmetric ...
Raziyeh Zaregonbadi +2 more
doaj +1 more source
Indefinitely Flat Circular Velocities and the Baryonic Tully–Fisher Relation from Weak Lensing
We use a new deprojection formula to infer the gravitational potential around isolated galaxies from weak gravitational lensing. The results imply circular velocity curves that remain flat for hundreds of kiloparsecs, greatly extending the classic result
Tobias Mistele +4 more
doaj +1 more source
The Survival of the Sagittarius Dwarf Galaxy and the Flatnessof the Rotation Curve of the Galaxy [PDF]
Hongsheng Zhao
openalex +1 more source
Discs no more: the morphology of low-mass simulated galaxies in FIREbox. [PDF]
Benavides JA +11 more
europepmc +1 more source
Gravitational Hamiltonian Systems and the Retarded Gravity Inequality. [PDF]
Yahalom A.
europepmc +1 more source
A giant disk galaxy two billion years after the Big Bang. [PDF]
Wang W +16 more
europepmc +1 more source

