Journal article icon

Journal article

Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations

Abstract:

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 the dependence of these mass functions on environment and redshift. The two methods also make similar predictions for the galaxy content of dark matter haloes as a function of halo mass and for the...

Expand abstract
Publication status:
Published

Actions


Access Document


Authors


Expand authors...
Journal:
Mon.Not.Roy.Astron.Soc.
Volume:
377
Issue:
1
Pages:
63-76
Publication date:
2006-05-31
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
URN:
uuid:dd14fa2f-8959-4c1a-a5d7-eef23d2fe8c6
Source identifiers:
205714
Local pid:
pubs:205714
Language:
English
Keywords:

Terms of use


Metrics


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP