Publication Date
1998
Journal or Book Title
Highly Redshifted Radio Lines
Abstract
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 maWe 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.ss functions and galaxy correlation functions could be used to discriminate between different cosmological models.
Pages
1
Volume
156
Recommended Citation
Katz, N; Hernquist, L; and Weinberg, DH, "Simulating Gas at High Redshift" (1998). Highly Redshifted Radio Lines. 982.
Retrieved from https://scholarworks.umass.edu/astro_faculty_pubs/982
Comments
This is the pre-published version harvested from ArXiv. The published version is located at http://www.aspbooks.org/a/volumes/article_details/?paper_id=16598