Modeling high-redshift galaxies: what can we learn from high and ultra-high resolution hydrodynamica...
Modeling high-redshift galaxies: what can we learn from high and ultra-high resolution hydrodynamical simulations?
About this item
Full title
Author / Creator
Devriendt, J. , Slyz, A. , Powell, L. , Pichon, C. and Teyssier, R.
Publisher
Cambridge, UK: Cambridge University Press
Journal title
Language
English
Formats
Publication information
Publisher
Cambridge, UK: Cambridge University Press
Subjects
More information
Scope and Contents
Contents
We present results from a high resolution cosmological galaxy formation simulation called Mare Nostrum and a ultra-high resimulation of the first 500 million years of a single, Milky Way (MW) sized galaxy. Using the cosmological run, we measure UV luminosity functions and assess their sensitivity to both cosmological parameters and dust extinction....
Alternative Titles
Full title
Modeling high-redshift galaxies: what can we learn from high and ultra-high resolution hydrodynamical simulations?
Authors, Artists and Contributors
Author / Creator
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_miscellaneous_745630933
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_745630933
Other Identifiers
ISSN
1743-9213
E-ISSN
1743-9221
DOI
10.1017/S1743921310002863
