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Dependence of Star Formation Rate on Overdensity

Kentaro Nagamine·Renyue Cen·Jeremiah P. Ostriker
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Abstract

We use a large-scale Lambda-CDM hydrodynamical simulation to assess the dependence of the cosmic Star Formation Rate (SFR) on overdensity of luminosity. The `morphology-density relation' is qualitatively captured when the SFR is plotted as a function of redshift, divided into the quartiles of the overdensity distribution.

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Kentaro Nagamine, Renyue Cen, Jeremiah P. Ostriker. 2003-11-13. Dependence of Star Formation Rate on Overdensity. https://arxiv.org/abs/astro-ph/9912023

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