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...
المؤلفون الرئيسيون: | Kraljic, K, Pichon, C, Codis, S, Laigle, C, Davé, R, Dubois, Y, Hwang, HS, Pogosyan, D, Arnouts, S, Devriendt, J, Musso, M, Peirani, S, Slyz, A, Treyer, M |
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التنسيق: | Journal article |
اللغة: | English |
منشور في: |
Oxford University Press
2019
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مواد مشابهة
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منشور في: (2016) -
Intrinsic alignment of simulated galaxies in the cosmic web: implications for weak lensing surveys
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منشور في: (2015) -
The Horizon-AGN simulation: evolution of galaxy properties over cosmic time
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