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19 April 2024
 
  » arxiv » astro-ph/0311294

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Is There a Missing Galaxy Problem at High Redshift?
Kentaro Nagamine ; Renyue Cen ; Lars Hernquist ; Jeremiah P. Ostriker ; Volker Springel ;
Date 13 Nov 2003
Journal Astrophys.J. 610 (2004) 45-50
Subject astro-ph
Affiliation2,3), Volker Springel ( Harvard-CfA, Princeton, IoA Cambridge, MPA
AbstractWe study the evolution of the global stellar mass density in a Lambda cold dark matter universe using two different types of hydrodynamical simulations (Eulerian TVD and SPH) and the analytical model of Hernquist & Springel (2003). We find that the theoretical calculations all predict both a higher stellar mass density at z~3 than indicated by current observations, and that the peak of the cosmic star formation rate history should lie at z~5. Such a star formation history implies that as much as (70%, 30%) of the total stellar mass density today must already have formed by z=(1, 3). Our results suggest that current observations at z~3 are missing as much as 50% of the total stellar mass density in the Universe, perhaps owing to an inadequate allowance for dust obscuration in star-forming galaxies, limited sample sizes, or cosmic variance. We also compare our results with some of the updated semi-analytic models of galaxy formation.
Source arXiv, astro-ph/0311294
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