Journal
ASTROPHYSICAL JOURNAL
Volume 550, Issue 2, Pages L129-L132Publisher
UNIV CHICAGO PRESS
DOI: 10.1086/319644
Keywords
cosmology : theory; large-scale structure of universe
Categories
Ask authors/readers for more resources
Recently there has been a lot of attention focused on a virialized halo-based approach to understanding the properties of the matter and galaxy power spectrum. A key ingredient in this model is the number and distribution of galaxies within dark matter halos as a function of mass. This quantity has been predicted from semianalytic modeling and from fits to observational data. Here we present predictions for the occupation number and spatial distribution of subhalos based on a high-resolution hydrodynamical simulation including cooling, star formation, and feedback.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available