Results 121 to 130 of about 2,129 (213)
Recent measurements of the Milky Way rotation curve found a sharp decline at around 15–20 kpc from the center of the Galaxy, suggesting that the Galactic dark matter halo is much less massive than predicted by other dynamical tracers.
Xiaowei Ou +5 more
doaj +1 more source
Newtonian Gravity and Galaxy Rotation Curves: An Axisymmetric Green's Function Perspective [PDF]
The standard proposal within the context of General relativity and its weak field Newtonian limit for the nature of dark matter is that it consists of dark matter particles of unknown type.
Govaerts, Jan
core +2 more sources
The Nearly Universal Disk Galaxy Rotation Curve
The universal rotation curve (URC) of disk galaxies was originally proposed to predict the shape and amplitude of any rotation curve (RC) based solely on photometric data.
Raj Patel +5 more
doaj +1 more source
Perfect fluid dark matter: a viability test with galaxy rotation curves
The anomalous rotation curves of galaxies provide compelling evidence for dark matter, yet its fundamental nature and distribution remain key unresolved issues in astrophysics.
Jan Kuncewicz
doaj +1 more source
We characterize stellar, gas, and dark matter mass distributions for 17 nearby massive disk galaxies from the PHANGS sample. This allows us to compute the gravitational potential that vertically confines the interstellar gas and determines its ...
Vivek Vijayakumar +7 more
doaj +1 more source
Declining rotation curves in interacting galaxies [PDF]
A declining rotation curve was recently found for the galaxy NGC 3521 by HI synthesis telescope observations (Casertano and van Gorkom 1991). From a comparison of the shapes of rotation curves for a larger sample of galaxies Casertano and van Gorkom ...
Dettmar, Ralf-Juergen, Skiff, Brian A.
core +1 more source
The free electron model with Boltzmann statistics for spherical low-density plasmas is developed further, with asymptotic relations obtaining the density of electrons, mass densities, and the potentials of such plasmas.
Y. Ben-Aryeh
doaj +1 more source
We use the IllustrisTNG cosmological hydrodynamical simulation to study the rotation curves of galaxies in the local universe. To do that, we first select the galaxies with 9.4
Daeun Jeong +3 more
doaj +1 more source
A unique galaxy at z = 2.2, zC406690, has a striking clumpy large-scale ring structure that persists from rest-frame UV to near-infrared, yet has an ordered rotation and lies on the star formation main sequence.
A. Nestor Shachar +26 more
doaj +1 more source
Optical Rotation Curves Of Distant Galaxies : [PDF]
ng V and I photometry, disk and bulge deconvolutions, and galaxy type, orientation, and inclination) have been observed with the Low Resolution Imaging Spectrograph (LRIS) on the Keck 10m telescope.
N. P. Vogt +2 more
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