The formation and survival of discs in a ΛcDM universe
We study the formation of galaxies in a Λ cold dark matter (ΛCDM) universe using high-resolution hydrodynamical simulations with a multiphase treatment of gas, cooling and feedback, focusing on the formation of discs. Our simulations follow eight isolated haloes similar in mass to the Milky Way and...
Guardado en:
Autores principales: | Scannapieco, C., White, S.D.M., Springel, V., Tissera, P.B. |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00358711_v396_n2_p696_Scannapieco |
Aporte de: |
Ejemplares similares
-
The formation and survival of discs in a ΛcDM universe
Publicado: (2009) -
Effects of supernova feedback on the formation of galaxy discs
por: Scannapieco, C., et al. -
Formation history, structure and dynamics of discs and spheroids in simulated Milky Way mass galaxies
por: Scannapieco, C., et al. -
Milky Way type galaxies in a ΛcDM cosmology
por: De Rossi, M.E., et al. -
Milky Way type galaxies in a ΛcDM cosmology
Publicado: (2009)