Results 61 to 70 of about 466,777 (152)
Bar Formation and Destruction in the FIRE-2 Simulations
The physical mechanisms responsible for bar formation and destruction in galaxies remain a subject of debate. While we have gained valuable insight into how bars form and evolve from isolated idealized simulations, in the cosmological domain, galactic ...
Sioree Ansar +7 more
doaj +1 more source
The Stellar Bar–Dark Matter Halo Connection in the TNG50 Simulations
Stellar bars in disk galaxies grow as stars in near-circular orbits lose angular momentum to their environments, including their dark matter (DM) halo, and transform into elongated bar orbits.
Sioree Ansar, Mousumi Das
doaj +1 more source
Clusters can provide propitious environments for bar formation in galaxies. This work studies the formation and evolution of 15 bar-like galaxies in the most massive cluster of the TNG50 simulation from the IllustrisTNG suite.
Łokas Ewa L.
doaj +1 more source
Galaxy And Mass Assembly (GAMA) : galaxy close pairs, mergers and the future fate of stellar mass [PDF]
ASGR acknowledges STFC and SUPA funding that were used to do this work. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO and the participating institutions.We use a highly complete subset of the Galaxy And Mass Assembly II (GAMA-II) redshift
De Propris, R. +130 more
core +1 more source
Galaxy Zoo CEERS: Bar Fractions Up to z ∼ 4.0
We study the evolution of the bar fraction in disk galaxies between 0.5
Tobias Géron +24 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
Cyclic response of RC beam-column joints reinforced with plain bars: an experimental testing campaign [PDF]
Existing reinforced concrete (RC) buildings constructed until the mid-70’s, with plain reinforcing bars, are expected to behave poorly when subjected to earthquake actions.
Costa, A. +3 more
core
The Hot and Energetic Universe:The evolution of galaxy groups and clusters [PDF]
Major astrophysical questions related to the formation and evolution of structures, and more specifically of galaxy groups and clusters, will still be open in the coming decade and beyond: what is the interplay of galaxy, supermassive black hole, and ...
Bourdin, H. +47 more
core
BackofenLab/docker-galaxy-graphclust: Initial release
Galaxy flavor for ...
Milad Miladi +2 more
core +1 more source
Connection between Nonaxisymmetric Structures and Neutral Gas Distribution in Disk Galaxies
Nonaxisymmetric structures, such as bars and spiral arms, are known to concentrate molecular gas and star formation in galaxy centers, actively building up the pseudobulges.
Ze-Zhong Liang +4 more
doaj +1 more source

