Results 81 to 90 of about 198 (153)
We analyze bars formed in N -body simulations to investigate two key aspects of stellar kinematic structure of barred galaxies: the angular distributions of the radial and azimuthal components of stellar velocities, and the impact of bars on rotation ...
Seungwon Baek +3 more
doaj +1 more source
Simulations of cosmic ray propagation. [PDF]
Hanasz M, Strong AW, Girichidis P.
europepmc +1 more source
Discovery of a Barred-spiral Galaxy at zspec = 3.16. II. The Star Formation History
We present a detailed analysis of a massive barred galaxy at z _spec = 3.1591 using deep multiband imaging from the Hubble Space Telescope (HST) and JWST.
Yingjie Cheng +8 more
doaj +1 more source
Light reprocessed by dust grains emitting in the infrared enables the study of the physics at play in dusty embedded regions, where ultraviolet and optical wavelengths are attenuated.
Ramambason Lise +34 more
doaj +1 more source
Galactic Bars Are Already Mature at Cosmic Noon: Bar Strength and Flatness at z ∼ 1.5
In this work, we explore the nature of z > 1 galactic bars. Once thought to be highly transient, our results demonstrate otherwise. Our sample consists of nine massive (>10 ^10.5 M _⊙ ) star-forming barred-spiral galaxies at z _spec ∼ 1.5.
Boris S. Kalita +8 more
doaj +1 more source
Noncircular (NC) motions have been observed across various spatial scales in disk galaxies, yet the physical properties of the gas involved in these motions remain poorly constrained.
Carlos López-Cobá +6 more
doaj +1 more source
Multiscale Gas Structure and Dynamics in an Extragalactic Central Molecular Zone
The structures and dynamics of the interstellar medium are governed by a combination of self-gravity, external gravity, and various sources of ordered and random motions on different spatial scales.
Liam M. Wang +6 more
doaj +1 more source
Discovery of diffuse optical emission lines from the inner Galaxy: Evidence for LI(N)ER-like gas. [PDF]
Krishnarao D, Benjamin RA, Haffner LM.
europepmc +1 more source
ALMA-LEGUS. II. The Influence of Subgalactic Environments on Molecular Cloud Properties
We compare the molecular cloud properties in subgalactic regions of two galaxies, barred spiral NGC 1313, which is forming many massive clusters, and flocculent spiral NGC 7793, which is forming significantly fewer massive clusters despite having a ...
Molly K. Finn +26 more
doaj +1 more source
Automated Detection of Galactic Rings from Sloan Digital Sky Survey Images
Morphological features in galaxies—like spiral arms, bars, rings, and tidal tails, etc.—carry information about their structure, origin, and evolution.
Linn Abraham +6 more
doaj +1 more source

