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The formation of galaxies

New Astronomy Reviews, 2001
Abstract The basic framework for a successful theory of large-scale structure is provided by the cold dark matter hypothesis. It works surprisingly well, and has led to predictions, such as the clustering of gas and galaxies as a function of redshift, that have been observationally tested.
Joseph Silk, Rychard Bouwens
openaire   +1 more source

Formation of the Galaxy

Symposium - International Astronomical Union, 1967
From observations it is deduced that the disk and halo were formed about the same time and that most of the previously gaseous Galaxy became stars then. Dimensional analysis indicates that the flattening of a galaxy is related to its energy,E, angular momentum,H, and mass,M, by the dimensionless number - 2EH2/G5M5.
openaire   +1 more source

The Formation of the Galaxy

1987
The formation of galaxies from density perturbations is discussed, and it is shown that the Galaxy could have grown from a typical isolated peak in the now-fashionable “cold dark matter” model; most of its properties are correctly predicted by such a model.
openaire   +1 more source

Formation of a spiral galaxy

ACM SIGGRAPH 2007 computer animation festival, 2007
openaire   +1 more source

Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter

Monthly Notices of the Royal Astronomical Society, 2022
Alis J Deason   +2 more
exaly  

SEAGLE – II. Constraints on feedback models in galaxy formation from massive early-type strong-lens galaxies

Monthly Notices of the Royal Astronomical Society, 2021
Sampath Mukherjee   +2 more
exaly  

Galaxy formation in the Santa Cruz semi-analytic model compared with IllustrisTNG – I. Galaxy scaling relations, dispersions, and residuals at z = 0

Monthly Notices of the Royal Astronomical Society, 2022
Austen Gabrielpillai   +2 more
exaly  

Massive galaxy formation caught in action at z ∼ 5 with JWST

Astronomy and Astrophysics, 2023
S Jin, Nikolaj B Sillassen, G Magdis
exaly  

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