Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
The interplay of star formation (SF) and supernova (SN) feedback in galaxy formation is a key element for understanding galaxy evolution. Since these processes occur at small scales, it is necessary to have sub-grid models that recover their evolution and environmental effects at the scales reached...
Autors principals: | Nuñez-Castiñeyra, A, Nezri, E, Devriendt, J, Teyssier, R |
---|---|
Format: | Journal article |
Idioma: | English |
Publicat: |
Oxford University Press
2020
|
Ítems similars
-
Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics
per: Nuñez-Castiñeyra, A, et al.
Publicat: (2023) -
The radius of baryonic collapse in disc galaxy formation
per: Kassin, SA, et al.
Publicat: (2012) -
The radius of baryonic collapse in disc galaxy formation
per: Kassin, SA, et al.
Publicat: (2012) -
Modelling baryonic feedback for survey cosmology
per: Elisa Chisari, et al.
Publicat: (2019-06-01) -
Modelling baryonic feedback for survey cosmology
per: Elisa Chisari, et al.
Publicat: (2019-06-01)