Results 161 to 170 of about 30,211 (248)

Rings and spirals in barred galaxies â II. Ring and spiral morphology [PDF]

open access: bronze, 2009
E. Athanassoula   +3 more
openalex   +1 more source

The H i morphology and stellar properties of strongly barred galaxies: support for bar quenching in massive spirals [PDF]

open access: bronze, 2020
Lucy Claire Newnham   +6 more
openalex   +1 more source

Gas Streaming in Barred Spiral Galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1965
K. C. Freeman, L. Mestel
openaire   +1 more source

Hidden Gems on a Ring: Infant Massive Clusters and Their Formation Timeline Unveiled by ALMA, HST, and JWST in NGC 3351

open access: yesThe Astrophysical Journal
We use 0.1″ observations from the Atacama Large Millimeter Array (ALMA), Hubble Space Telescope (HST), and JWST to study young massive clusters (YMCs) in their embedded “infant” phase across the central starburst ring in NGC 3351.
Jiayi Sun   +40 more
doaj   +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

THE CENTRAL REGION OF THE BARRED SPIRAL GALAXY NGC 1097 PROBED BY AKARI NEAR-INFRARED SPECTROSCOPY [PDF]

open access: bronze, 2012
T. Kondo   +8 more
openalex   +1 more source

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

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