CLUSTERS OF SMALL CLUMPS CAN EXPLAIN THE PECULIAR PROPERTIES OF GIANT CLUMPS IN HIGH-REDSHIFT GALAXIES
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8205/819/1/L2/pdf
Reference46 articles.
1. Disc formation and the origin of clumpy galaxies at high redshift
2. THE STRUCTURE OF GRAVITATIONALLY UNSTABLE GAS-RICH DISK GALAXIES
3. DYNAMO – II. Coupled stellar and ionized-gas kinematics in two low-redshift clumpy discs
4. Structure formation in gas-rich galactic discs with finite thickness: from discs to rings
5. Towards a more realistic sink particle algorithm for the ramses code
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