Results 21 to 30 of about 957 (185)
We report VLA B-configuration observations of the H i 21 cm line on the close disk galaxy pair NGC 5595 and NGC 5597. At the angular resolution of the observations, ∼7.″1 × 4.″2, while most of the H i 21 cm in NGC 5595 and NGC 5597 has the same extent as
J. Antonio Garcia-Barreto +1 more
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Testing universal dark-matter caustic rings with galactic rotation curves
Infall of cold dark matter on a galaxy may result in caustic rings where the particle density is enhanced. They may be searched for as features in the galactic rotation curves.
Daniil Davydov, Sergey Troitsky
doaj +1 more source
Galactic rotation dynamics in a new $$f({\mathcal {R}})$$ f ( R ) gravity model
We propose to test the viability of the recently introduced $$f(\mathcal {R})$$ f ( R ) gravity model in the galactic scales. For this purpose we consider test particles moving in stable circular orbits around the galactic center.
Nashiba Parbin, Umananda Dev Goswami
doaj +1 more source
Conformally-rescaled Schwarzschild metrics do not predict flat galaxy rotation curves
For conformally invariant gravity theories defined on Riemannian spacetime and having the Schwarzschild–de-Sitter (SdS) metric as a solution in the Einstein gauge, we consider whether one may conformally rescale this solution to obtain flat rotation ...
Michael Hobson, Anthony Lasenby
doaj +1 more source
On the Keplerian Rotation Curves of Galaxies [PDF]
We propose a criterion for examining whether or not the uncertainty of the outer rotation curves is sufficiently small to distinguish a Keplerian rotation curve from flat ones. We have applied this criterion to both Keplerian and non-Keplerian rotation curves so far obtained, and investigated their relative fraction.
Honma, Mareki, Sofue, Yoshiaki
openaire +2 more sources
Rotation curve of our Galaxy and field galaxies [PDF]
We present a database of galaxies rotation curve (from Hα observations), including our Galaxy.
D. Russeil +3 more
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Galaxy rotation curves and preferred reference frame effects
As an alternative to dark matter models we use generalized Jordan–Brans–Dicke scalar–vector–tensor (JBD-SVT) gravity model to study the behavior of the rotational velocities of test particles moving around galaxies.
Hossein Ghaffarnejad, Razieh Dehghani
doaj +1 more source
The universal rotation curve of dwarf disc galaxies [PDF]
We use the concept of the spiral rotation curves universality to investigate the luminous and dark matter properties of the dwarf disc galaxies in the local volume (size $\sim11$ Mpc). Our sample includes 36 objects with rotation curves carefully selected from the literature.
Karukes E. V., Salucci P.
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The unexpected diversity of dwarf galaxy rotation curves [PDF]
17 pages, 6 figures, 2 tables, MNRAS ...
Oman, K.A. +11 more
openaire +8 more sources
Rotation curves of galaxies in GR
It has been suggested that the observed flat rotation curves of disk galaxies can be a peculiar effect of General Relativity (GR) rather than evidence for the presence of dark matter (DM) halos in Newtonian gravity. In Ciotti (2022) the problem has been quantitatively addressed by using the well known weak-field, low-velocity gravitomagnetic limit of ...
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