The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes
We investigate the impact of the number of filaments connected to the nodes of the cosmic web on the physical properties of their galaxies using the Sloan Digital Sky Survey. We compare these measurements to the cosmological hydrodynamical simulations Horizon-(no)AGN and Simba. We find that more mas...
主要な著者: | , , , , , , , , , , , , , |
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フォーマット: | Journal article |
言語: | English |
出版事項: |
Oxford University Press
2019
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