Prevalent elongated galaxies in the early Universe evidenced by stellar kinematics
Bitao Wang, Yingjie Peng, and Hua Gao

TL;DR
This study uses stellar kinematics to show that early low-mass galaxies in the Universe were predominantly elongated prolate ellipsoids, indicating a fundamental morphological transition from spindle-like to disc-shaped galaxies over cosmic time.
Contribution
It provides the first decisive evidence supporting the prolate spindle morphology of high-redshift galaxies through stellar kinematics analysis.
Findings
Early Universe galaxies are mainly elongated prolate ellipsoids.
A dimensional transition from prolate to disc morphology occurred over cosmic time.
Supports the idea of morphological evolution in galaxy structure.
Abstract
The Universe is now extensively populated by discy galaxies with coherent galaxy-wise stellar rotation. This disc prevalence has been deemed a late-time phenomenon because the penetrating cold gaseous streams in the early Universe () fuel the star formation in galaxies too intensively to allow for thin disc formation. However, recent images taken by the James Webb Space Telescope (JWST) unveiled a prominent population of low-mass galaxies at high redshifts with flattened shapes, widely interpreted as early significance of discs given the well-established connection between flattening and discy morphology seen in the local Universe. It is noticed, on the other hand, that these galaxies show far more flattened systems than can be accounted for by randomly oriented oblate discs, and the axial ratio distributions are better explained by elongated prolate ellipsoids, an extremely…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Electrical and Electromagnetic Research
