The Cosmic Web of Baryons

TL;DR

This paper discusses the Cosmic Web of baryons, emphasizing the importance of X-ray observations to detect and analyze the hot, diffuse gas that constitutes most of the universe's baryonic matter outside galaxies.

Contribution

It highlights the potential of future X-ray telescopes like IXO to test key predictions about the distribution, dynamics, and topology of baryonic gas in the Cosmic Web.

Findings

Most baryons are in hot, diffuse filaments detectable via X-ray absorption and emission.

X-ray observations can reveal the distribution and temperature of the gas.

The topology of the Cosmic Web can be mapped through these observations.

Abstract

Only about 10% of the baryons in the universe lie in galaxies as stars or cold gas, with the remainder predicted to exist as a dilute gaseous filamentary network known as the Cosmic Web. Some of this gas is detected through UV absorption line studies, but half of the gas remains undetected. Growth of structure simulations suggest that these "missing" baryons were shock heated in unvirialized cosmic filaments to temperatures of 10^5.5-10^7 K, and that the gas is chemically enriched by galactic superwinds. Most of the gas in this temperature regime can be detected only by X-ray observations through absorption and emission from the He-like and H-line ions of C, N, and O. This white paper shows that an X-ray telescope such as IXO can test the most central predictions of the Cosmic Web: the distribution of gas mass with temperature; the dynamics of the gas and its relationship to nearby galaxies; and the topology of the Cosmic Web material.