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- W2006314686 abstract "We examine the correlation property of Lyα forest (along the line of sight) utilizing a hydrodynamic simulation of Lyα clouds in a cold dark matter universe with a cosmological constant, and compare it to the correlation of underlying mass and galaxies. A consistent picture seems to emerge: the correlation strength for a given set of objects is positively correlated with their characteristic global density and the differences among the correlations of galaxies, Lyα clouds, and mass reflect the differences in density that each trace. We find that the galaxies are strongly biased (nearly independent of scales) over mass by a factor of ~3.0, in accord with recent observations of high-redshift galaxies. The correlation strength of Lyα clouds with column densities of 1013-1014 cm-2 is comparable to that of total mass. Positive correlations with a strength of 0.1-1.0 are found for Lyα clouds in the velocity range 50-300 km s-1. The correlation is less than 0.3 at Δv > 300 km s-1, but here our simulated box is too small to give a reliable measure." @default.
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- W2006314686 date "1998-04-01" @default.
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- W2006314686 title "On the Clustering of Lyα Clouds, High‐Redshift Galaxies, and Underlying Mass" @default.
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