Results 71 to 80 of about 198 (153)

A Milky Way-like barred spiral galaxy at a redshift of 3. [PDF]

open access: yesNature, 2023
Costantin L   +32 more
europepmc   +1 more source

Perspectives. [PDF]

open access: yesAJNR Am J Neuroradiol, 2023
Ross JS.
europepmc   +1 more source

Orbital Classification in Rotating Bar Potentials Using an Empirical Proxy of the Second Integral of Motion

open access: yesThe Astrophysical Journal
We present a novel method for classifying two-dimensional orbits in rotating bar potentials based on an empirical proxy for the second integral of motion, calibrated angular momentum (CAM), which is defined as the ratio of the time-averaged angular ...
Tian-Ye Xia   +3 more
doaj   +1 more source

A Stellar Bar Hidden in an Extreme Gas-rich Disk Galaxy at z = 4.055

open access: yesThe Astrophysical Journal Letters
The classical picture for the formation of stellar bars—key dynamical drivers of the evolution of galaxies—is through secular evolution of instability in gas-poor, stellar-dominated disks. The detection with the James Webb Space Telescope of stellar bars
Leindert A. Boogaard   +16 more
doaj   +1 more source

Identification and Analysis of Galactic Bars in DESI Legacy Imaging Surveys

open access: yesThe Astrophysical Journal
We present a comprehensive study of bar structures in the local universe using data from the DESI Legacy Imaging Surveys. Through isophotal analysis of 232,142 galaxies, we identify bars and classify them into strong and weak categories based on ...
Wenwen Wang, Zhimin Zhou
doaj   +1 more source

Impacts of Bar-driven Shear and Shocks on Star Formation

open access: yesThe Astrophysical Journal
Bars drive gas inflow. As the gas flows inward, shocks and shear occur along the bar dust lanes. Such shocks and shear can affect the star formation (SF) and change the gas properties.
Taehyun Kim   +14 more
doaj   +1 more source

Formation Mechanisms for Spirals in Barred Galaxies

open access: yes, 2000
We consider a scenario of formation of the spiral structure in barred galaxies. This scenario includes the new non-resonant mechanism of elongation of spirals, due to the characteristic behaviour of the gravitational potential beyond the principal spiral arms.
Polyachenko, Evgenii V.   +1 more
openaire   +2 more sources

Do Strong Bars Exhibit Strong Noncircular Motions?

open access: yesThe Astrophysical Journal
Galactic bars induce characteristic motions deviating from pure circular rotation, known as noncircular motions. As bars are nonaxisymmetric structures, stronger bars are expected to show stronger noncircular motions.
Taehyun Kim   +6 more
doaj   +1 more source

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