Results 131 to 140 of about 64,819 (265)
The mass distribution in early-type disc galaxies: declining rotation curves and correlations with optical properties [PDF]
E. Noordermeer +4 more
openalex +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
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
GHASP. A 3D Survey of Spiral and Irregular Galaxies at Halpha. Comparison between low and high resolution rotation curves of late-type dwarf galaxies [PDF]
P. Amram, O. Garrido
openalex +1 more source
Dark Matter and Rotation Curves of Stars in Galaxies [PDF]
Ernst Schmützer
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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
Rotation curves of high-resolution LSB and SPARC galaxies with fuzzy and multistate (ultralight boson) scalar field dark matter [PDF]
Tula Bernal +3 more
openalex +1 more source
The Impact of Bar-induced Noncircular Motions on the Measurement of Galactic Rotation Curves
We study the impact of bar-induced noncircular motions on the derivation of galactic rotation curves (RCs) using hydrodynamic simulations and observational data from the PHANGS-ALMA survey.
Jie Liu, Zhi Li, Juntai Shen
doaj +1 more source
Recent evidence on the rotation curve of our galaxy for R > RO [PDF]
P. Jackson +2 more
openalex +1 more source
Low-surface-brightness galaxies are excellent laboratories, where stars and baryonic matter act as tracers of the gravitational potential of the dark matter halo.
A. Aceña +4 more
doaj +1 more source

