X-ray Observations of the Warm-Hot Intergalactic Medium

Mathematics – Logic

Scientific paper

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Scientific paper

Most of the baryons in the low-redshift Universe appear to be missing. Hydrodynamic cosmological simulations predict that they reside in the intergalactic medium which has been shock-heated to millions of degrees. Such warm-hot intergalactic medium is observable through X-ray absorption lines in the spectra of background quasars. I will describe our work on finding the missing baryons with the Chandra X-ray Observatory.

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