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The evolution of galaxy structure over cosmic time
CJ Conselice - Annual Review of Astronomy and Astrophysics, 2014 - annualreviews.org
I present a comprehensive review of the evolution of galaxy structure in the Universe from
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …
Coevolution (or not) of supermassive black holes and host galaxies
J Kormendy, LC Ho - Annual Review of Astronomy and …, 2013 - annualreviews.org
Supermassive black holes (BHs) have been found in 85 galaxies by dynamical modeling of
spatially resolved kinematics. The Hubble Space Telescope revolutionized BH research by …
spatially resolved kinematics. The Hubble Space Telescope revolutionized BH research by …
The epoch of the Milky Way's bar formation: dynamical modelling of Mira variables in the nuclear stellar disc
JL Sanders, D Kawata, N Matsunaga… - Monthly Notices of …, 2024 - academic.oup.com
ABSTRACT A key event in the history of the Milky Way is the formation of the bar. This event
affects the subsequent structural and dynamical evolution of the entire Galaxy. When the bar …
affects the subsequent structural and dynamical evolution of the entire Galaxy. When the bar …
The rapid onset of stellar bars in the baryon-dominated centers of disk galaxies
J Bland-Hawthorn, T Tepper-Garcia… - The Astrophysical …, 2023 - iopscience.iop.org
Recent observations of high-redshift galactic disks (z≈ 1–3) show a strong negative trend in
the dark-matter (DM) fraction f DM with increasing baryon surface density. For this to be true …
the dark-matter (DM) fraction f DM with increasing baryon surface density. For this to be true …
Secular evolution and the formation of pseudobulges in disk galaxies
J Kormendy, RC Kennicutt Jr - Annu. Rev. Astron. Astrophys., 2004 - annualreviews.org
▪ Abstract The Universe is in transition. At early times, galactic evolution was dominated by
hierarchical clustering and merging, processes that are violent and rapid. In the far future …
hierarchical clustering and merging, processes that are violent and rapid. In the far future …
The existence and shapes of dust lanes in galactic bars
E Athanassoula - Monthly Notices of the Royal Astronomical …, 1992 - academic.oup.com
I study the flow of gas in and around the bars or ovals of model barred galaxies and show
that it is intimately linked to the properties of the periodic orbits. Simulations show that the …
that it is intimately linked to the properties of the periodic orbits. Simulations show that the …
Secular evolution in disk galaxies
JA Sellwood - Reviews of Modern Physics, 2014 - APS
Disk galaxies evolve over time through processes that may rearrange both the radial mass
profile and the metallicity distribution within the disk. This review of such slow changes is …
profile and the metallicity distribution within the disk. This review of such slow changes is …
Physical properties and environments of nearby galaxies
MR Blanton, J Moustakas - Annual Review of Astronomy and …, 2009 - annualreviews.org
We review the physical properties of nearby, relatively luminous galaxies, using results from
newly available massive data sets together with more detailed observations. First, we …
newly available massive data sets together with more detailed observations. First, we …
The evolution of the barred galaxy population in the TNG50 simulation
Y Rosas-Guevara, S Bonoli, M Dotti… - Monthly Notices of …, 2022 - academic.oup.com
We use the magnetic-hydrodynamical simulation TNG50 to study the evolution of barred
massive disc galaxies. Massive spiral galaxies are already present as early as z= 4, and bar …
massive disc galaxies. Massive spiral galaxies are already present as early as z= 4, and bar …
[HTML][HTML] Box and peanut shapes generated by stellar bars
F Combes, F Debbasch, D Friedli… - … , no. 1, July 1990, p. 82 …, 1990 - adsabs.harvard.edu
By means of three-dimensional N-body simulations, we find that all the stellar bars that
develop in realistic models of collisionless disk galaxies take after some time a more or less …
develop in realistic models of collisionless disk galaxies take after some time a more or less …