Results 111 to 120 of about 8,619 (233)

Do Strong Bars Exhibit Strong Noncircular Motions?

open access: yesThe Astrophysical Journal
Galactic bars induce characteristic motions deviating from pure circular rotation, known as noncircular motions. As bars are nonaxisymmetric structures, stronger bars are expected to show stronger noncircular motions.
Taehyun Kim   +6 more
doaj   +1 more source

A Milky Way-like barred spiral galaxy at a redshift of 3. [PDF]

open access: yesNature, 2023
Costantin L   +32 more
europepmc   +1 more source

Inner Molecular Rings in Barred Galaxies: BIMA SONG CO Observations

open access: yes, 2002
Although inner star-forming rings are common in optical images of barred spiral galaxies, observational evidence for the accompanying molecular gas has been scarce.
Buta R.   +9 more
core   +1 more source

Morphological Evolution of Disk Galaxies and Their Concentration, Asymmetry, and Clumpiness (CAS) Properties in Simulations across Toomre’s Q Parameter

open access: yesThe Astrophysical Journal
We investigate the morphological and structural evolution of disk galaxies in simulations for a wide range of Toomre’s Q parameters. In addition to the inspection of conventional bar modes, we compute the concentration, asymmetry, and clumpiness (CAS ...
T. Chantavat   +3 more
doaj   +1 more source

Orbital structure in barred spiral galaxies

open access: yes, 2010
15 pages, 20 ...
Harsoula, Maria   +1 more
openaire   +2 more sources

N-body Simulations of Galaxy Bars Generated by Satellite Collisions: Effects of the Impact Geometry

open access: yesThe Astrophysical Journal
Bars, a common and important structure in disk galaxies, can be induced by galaxy interactions. Although there have been some studies on bar formation in flybys or collisions, the vast parameter space still leaves many scenarios that require further ...
Yufan Fane Zhou, Zhiyuan Li, Hui Li
doaj   +1 more source

Is NGC 4631 a barred spiral galaxy?

open access: yesThe Astronomical Journal, 1991
High- and low-dispersion optical spectra of the giant H II region CM 67 near the center of the edge-on galaxy NGC 4631 have been obtained. Comparisons are made with radio observations to suggest the existence of a large bar in NGC 4631. Region CM 67 is shown to coincide in position with the easternmost peak of a triple radio-continuum source.
Jean-Rene Roy   +2 more
openaire   +1 more source

Dynamical Mechanism of Episodic Gas Accretion to the Central Region of Spiral Galaxies

open access: yesThe Astrophysical Journal
We performed N -body/smoothed particle hydrodynamics simulations of isolated spiral galaxies with various bulge-to-disk mass ratios ( M _bulge / M _disk ) from 0.02 to 0.2 to investigate mass transport from galactic scales (10 kpc) down to circumnuclear ...
Naomichi Yutani   +3 more
doaj   +1 more source

The Impact of Bar-induced Noncircular Motions on the Measurement of Galactic Rotation Curves

open access: yesThe Astrophysical Journal
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

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