Results 191 to 200 of about 553,808 (287)
On the Role of Noncircular Motions in MaNGA Galaxies. I. Global Properties
Noncircular (NC) motions represent the imprints of nonaxisymmetric structures in galaxies, providing opportunities to study the physical properties of gas departing from circular rotation.
Carlos López-Cobá +3 more
doaj +1 more source
The Intrinsic Flattening of Galaxy Disks
Highly inclined (edge-on) disk galaxies offer the unique perspective to constrain their intrinsic flattening, c / a , where c and a are, respectively, the vertical and long radial axes of the disk measured at suitable stellar densities.
Jeremy Favaro +3 more
doaj +1 more source
Compact groups (CGs) of galaxies are dense systems where projected separations are comparable to their optical diameters. A subset—non-isolated CGs—are embedded within major structures. Using multiband S-PLUS data, we analyse galaxies in 122 non-isolated
Gissel P. Montaguth +19 more
doaj +1 more source
Galaxy Spin Alignment with Tidal Fields in the SDSS-IV MaNGA Survey
The tidal torque theory (TTT) predicts that galaxy spins are correlated with the surrounding tidal field, reflecting how angular momentum is acquired during structure formation.
Jun-Sung Moon, Teppei Okumura
doaj +1 more source
Indefinitely Flat Circular Velocities and the Baryonic Tully–Fisher Relation from Weak Lensing
We use a new deprojection formula to infer the gravitational potential around isolated galaxies from weak gravitational lensing. The results imply circular velocity curves that remain flat for hundreds of kiloparsecs, greatly extending the classic result
Tobias Mistele +4 more
doaj +1 more source
Utilizing the COSMOS H I Large Extragalactic Survey (CHILES) data set, we investigate the evolution of the average atomic neutral hydrogen (H I ) properties of galaxies over the continuous redshift range 0.09
Nicholas Luber +11 more
doaj +1 more source
Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations
In this study, we investigate the morphology of galaxies in the TNG100 simulation by applying mock observation techniques and compare the results with the observational data from the Sloan Digital Sky Survey (SDSS).
Jun-Yu Gong +3 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
A rising tide: intrinsic alignments since the turn of the millennium. [PDF]
Chisari NE.
europepmc +1 more source

