Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations
We compare the galaxy population of an SPH simulation to those predicted by the GalICS semi-analytic model and a stripped down version without supernova and AGN feedback. The SPH simulation and the no-feedback GalICS model make similar predictions for the baryonic mass functions of galaxies and for...
Huvudupphovsmän: | Cattaneo, A, Blaizot, J, Weinberg, D, Colombi, S, Dave, R, Devriendt, J, Guiderdoni, B, Katz, N, Keres, D |
---|---|
Materialtyp: | Journal article |
Språk: | English |
Publicerad: |
2006
|
Liknande verk
Liknande verk
-
Predicting multi-wavelength properties of Lyman break galaxies with GalICS
av: Blaizot, J, et al.
Publicerad: (2003) -
GalICS V : Low and high order clustering in mock SDSS's
av: Blaizot, J, et al.
Publicerad: (2006) -
GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback, and their roles in galaxy formation
av: Cattaneo, A, et al.
Publicerad: (2020) -
The new semi-analytic code GalICS 2.0 – reproducing the galaxy stellar mass function and the Tully–Fisher relation simultaneously
av: Cattaneo, A, et al.
Publicerad: (2017) -
GalICS II: the [alpha/Fe]-mass relation in elliptical galaxies
av: Pipino, A, et al.
Publicerad: (2008)