Results 111 to 120 of about 7,946 (225)
Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
We review internal processes of secular evolution in galaxy disks, concentrating on the buildup of dense central features that look like classical, merger-built bulges but that were made slowly out of disk gas. We call these pseudobulges. As an existence
Arp H +95 more
core +2 more sources
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
Astronomia ex machina: a history, primer and outlook on neural networks in astronomy. [PDF]
Smith MJ, Geach JE.
europepmc +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
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
Structure and dynamics of barred spiral galaxies with an asymmetric mass distribution [PDF]
G. de Vaucouleurs, K. C. Freeman
openalex +1 more source
Simulations of cosmic ray propagation. [PDF]
Hanasz M, Strong AW, Girichidis P.
europepmc +1 more source
We study the evolution of galactic bars and the link with disk and spheroid formation in a sample of zoom-in cosmological simulations. Our simulation sample focuses on galaxies with present-day stellar masses in the 10^10-10^11 Msun range, in field and ...
Aguerri +56 more
core +3 more sources
HI in the Barred Spiral Galaxies NGC 1365 and NGC 1097. [PDF]
J. M. van der Hulst +3 more
openalex +1 more source
Molecular gas in the central region of the starburst galaxy NGC 253 is complicated because of the combination of different gas kinematics, including stellar feedback, noncircular motions, and magnetic activity.
Ryotaro Konishi +5 more
doaj +1 more source

