A Combined HST/Chandra Study for Finding the Baryons in the Low Redshift Universe.

Mathematics – Logic

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Hst Proposal Id #10211 Quasar Absorption Lines/Igm

Scientific paper

The main reservoir of low redshift baryons is still ``missing'': All the observed stellar and gaseous components add up to a factor of ten below the abundance predicted by big bang nucleosynthesis. Hydrodynamic cosmological simulations predict that a large fraction of the low redshift baryons should reside in a warm/hot diffuse intergalactic medium {IGM}, detectable via an ``X-ray forest'' of high excitation metal lines, but blind searches of X-ray lines are extraordinarily difficult with present technology. A first hint of this warm-hot IGM may have been found in recent studies of OVI absorption towards background quasars. However, the significance of OVI absorbers to the total baryon budget is uncertain and UV observations alone cannot determine the physical conditions in the IGM. We propose STIS/E140M observations to search for intervening OVI absorbers towards two quasars that are bright enough in X-rays for follow-up Chandra spectroscopy. The combined UV/X-ray study provides a powerful tool to {1} assess the cosmological significance of OVI absorbers; {2} determine their physical properties using OVII/OVI and OVIII/OVI ratios; and {3} pursue detection and study of the warm-hot IGM.

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