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Gas Fraction Impact on Galactic Discs by jmsantos is a document available to read on EtoBox.
This study investigates the impact of gas fraction and stellar feedback on the stability and evolution of galactic discs, particularly focusing on the formation of giant clumps in high-redshift star-forming galaxies. The authors find that higher gas fractions lead to the formation of long-lived clumps, while gas-poor models produce short-lived clumps that are easily destroyed. The results suggest that many cosmological simulations may lack realistic gas fractions, contributing to the absence of giant clumps
- Author
- jmsantos
- Language
- EN