Simulating Gas at High Redshift
天体物理学
2007-05-23 v1
摘要
We discuss simulations of gas at high redshift. We briefly review the methods used and the results for quasar absorption lines. We present gas mass functions and galaxy correlation functions for 5 different cosmological models. Galaxies should be detectable at redshifts greater than 2 by SKAI, and measurements of the gas mass functions and galaxy correlation functions could be used to discriminate between different cosmological models.
关键词
引用
@article{arxiv.astro-ph/9801074,
title = {Simulating Gas at High Redshift},
author = {Neal Katz and Lars Hernquist and David H. Weinberg},
journal= {arXiv preprint arXiv:astro-ph/9801074},
year = {2007}
}
备注
9 pages, 4 figures in text, LaTex (paspconf.sty) To appear in the conference proceedings of Highly Redshifted Radio Lines