Results 111 to 120 of about 154,367 (172)
Properties of bars in the local universe [PDF]
We studied the fraction and properties of bars in a sample of about 3000 galaxies extracted from SDSS-DR5. This represents a volume limited sample with galaxies located between redshift 0.01
arxiv
The Clearing Timescale for Infrared-selected Star Clusters in M83 with HST
We present an analysis of Hubble Space Telescope data from Wide Field Camera 3 (WFC3)/Ultraviolet Imaging Spectrometer, WFC3/IR, and the Advanced Camera for Surveys, investigating the young stellar cluster (YSC) population in the face-on spiral galaxy ...
Suyash Deshmukh+8 more
doaj +1 more source
Orbital Support and Evolution of CX/OX Structures in Boxy/Peanut Bars
Barred galaxies exhibit boxy/peanut or X-shapes (BP/X) protruding from their disks in edge-on views. Two types of BP/X morphologies exist depending on whether the X-wings meet at the center (CX) or are off-centered (OX).
Behzad Tahmasebzadeh+9 more
doaj +1 more source
A Milky Way-like barred spiral galaxy at a redshift of 3 [PDF]
Luca Costantin+32 more
openalex +1 more source
Ring or No Ring—Revisiting the Multiphase Nuclear Environment in M31
Nuclear rings, prevalent in barred galaxies, are essential to understanding gas transport toward galactic nuclei. However, the peculiar nuclear ring in our neighboring galaxy M31 remains poorly understood.
Zongnan Li+11 more
doaj +1 more source
Thick disk and pseudobulge formation in a clump cluster
Bulges in spiral galaxies have been supposed to be classified into two types: classical bulges or pseudobulges. Classical bulges are thought to form by galactic merger with bursty star formation, whereas pseudobulges are suggested to form by secular ...
Inoue S.
doaj +1 more source
Bar-driven Transport of Molecular Gas in Spiral Galaxies: Observational Evidence [PDF]
The NRO-OVRO CO imaging survey showed that molecular gas was more concentrated to the central kiloparsec in barred spiral galaxies than in their unbarred counterparts. The result provided not only evidence for bar-driven gas transport but also estimates on the mean rate of gas transfer and lower limits to the lifetime of bars.
arxiv
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
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
Circumnuclear regions in barred spiral galaxies — I. Near-infrared imaging [PDF]
D. Pérez-Ramírez+5 more
openalex +1 more source