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Effect of Reionization on High-z Stellar Populations

  • Daniel Babich
Conference paper
Part of the Astrophysics and Space Science Proceedings book series (ASSSP)

Summary

I will discuss the effects of inhomogeneous reionization on the Spectral Energy Distributions (SED) of galaxies at high redshifts. The formation process of the ionizing sources is modulated by large scale density modes. This makes reionization inhomogeneous and introduces a spread to the reionization times of different regions with the same size. These scale-dependent fluctuations modify the shape of the power spectrum of low-mass galaxies at high redshifts in a way that depends on the history of reionization. High-mass galaxies are affected in a more subtle manner; their star formation histories depend on the local minimum mass of star formation. This produces changes in the SEDs of the galaxies.

Keywords

Dark Matter Star Formation High Redshift Star Formation Rate Spectral Energy Distribution 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag New York 2009

Authors and Affiliations

  1. 1.Theoretical Astrophysics California Institute of TechnologyPasadena

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