Results 21 to 30 of about 957 (185)

H i 21 cm Extended Structures to the Northeast and Southwest of NGC 5595: VLA Observations of the Disk Galaxy Pair NGC 5595 and NGC 5597

open access: yesThe Astronomical Journal, 2023
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
doaj   +1 more source

Testing universal dark-matter caustic rings with galactic rotation curves

open access: yesPhysics Letters B, 2023
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

open access: yesEuropean Physical Journal C: Particles and Fields, 2023
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

open access: yesEuropean Physical Journal C: Particles and Fields, 2022
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]

open access: yesPublications of the Astronomical Society of Japan, 1997
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]

open access: yesSymposium - International Astronomical Union, 2004
We present a database of galaxies rotation curve (from Hα observations), including our Galaxy.
D. Russeil   +3 more
openaire   +1 more source

Galaxy rotation curves and preferred reference frame effects

open access: yesEuropean Physical Journal C: Particles and Fields, 2019
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]

open access: yesMonthly Notices of the Royal Astronomical Society, 2016
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.
openaire   +4 more sources

The unexpected diversity of dwarf galaxy rotation curves [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
17 pages, 6 figures, 2 tables, MNRAS ...
Oman, K.A.   +11 more
openaire   +8 more sources

Rotation curves of galaxies in GR

open access: yes, 2023
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 ...
openaire   +2 more sources

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