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...
Autori principali: | Nuñez-Castiñeyra, A, Nezri, E, Devriendt, J, Teyssier, R |
---|---|
Natura: | Journal article |
Lingua: | English |
Pubblicazione: |
Oxford University Press
2020
|
Documenti analoghi
Documenti analoghi
-
Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics
di: Nuñez-Castiñeyra, A, et al.
Pubblicazione: (2023) -
The radius of baryonic collapse in disc galaxy formation
di: Kassin, SA, et al.
Pubblicazione: (2012) -
The radius of baryonic collapse in disc galaxy formation
di: Kassin, SA, et al.
Pubblicazione: (2012) -
Modelling baryonic feedback for survey cosmology
di: Elisa Chisari, et al.
Pubblicazione: (2019-06-01) -
Modelling baryonic feedback for survey cosmology
di: Elisa Chisari, et al.
Pubblicazione: (2019-06-01)