Dancing in the dark: galactic properties trace spin swings along the cosmic web
<p>A large-scale hydrodynamical cosmological simulation, Horizon-AGN, is used to investigate the alignment between the spin of galaxies and the cosmic filaments above redshift 1.2. The analysis of more than 150 000 galaxies per time step in the redshift range 1.2 < <em>z</em&g...
Үндсэн зохиолчид: | Dubois, Y, Pichon, C, Welker, C, Borgne, D, Devriendt, J, Laigle, C, Codis, S, Pogosyan, D, Arnouts, S, Benabed, K, Bertin, E, Blaizot, J, Bouchet, F, Cardoso, J, Colombi, S, Lapparent, V, Desjacques, V, Gavazzi, R, Kassin, S, Kimm, T, McCracken, H, Milliard, B, Peirani, S, Prunet, S, Rouberol, S, Silk, J, Slyz, A, Sousbie, T, Teyssier, R, Tresse, L, Treyer, M, Vibert, D, Volonteri, M |
---|---|
Формат: | Journal article |
Хэвлэсэн: |
Oxford University Press
2014
|
Ижил төстэй зүйлс
-
Swirling around filaments: are large-scale structure vortices spinning up dark haloes?
-н: Laigle, C, зэрэг
Хэвлэсэн: (2014) -
Intrinsic alignment of simulated galaxies in the cosmic web: implications for weak lensing surveys
-н: Codis, S, зэрэг
Хэвлэсэн: (2015) -
The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes
-н: Kraljic, K, зэрэг
Хэвлэсэн: (2019) -
Galaxy evolution in the metric of the Cosmic Web
-н: Kraljic, K, зэрэг
Хэвлэсэн: (2017) -
Connecting the cosmic web to the spin of dark halos: implications for
galaxy formation
-н: Codis, S, зэрэг
Хэвлэсэн: (2012)