Metallicity and D/H abundance in Low-z LyAlpha Absorbers towards PG 1211+143

Mathematics – Logic

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Hst Proposal Id #8571 Quasar Absorption Lines And Igm

Scientific paper

Our Cycle 7 STIS/G140M observations along the sightline toward PG 1211+143 reveal numerous LyAlpha absorption lines including 2 very strong LyAlpha absorbers {cz = 15, 300 and 19, 550 km s^- 1} with associated Si III absorption. These are the first definite detections of metals in a low-z LyAlpha forest cloud; simple photoionization models suggest metallicities in the range 1-10 sim10^17 cm^-2 in each system, we should be able to detect deuterium LyAlpha at 10-20 mAngstrom equivalent width, thereby testing models of D/H astration as a function of IGM metallicity, an issue of cosmological significance. We propose to obtain a 25-orbit {S/N 25} STIS/E140M spectrum {1150-1740 Angstrom} at 10 km s^-1 resolution to detect or limit D I {LyAlpha} and to measure metal absorption lines {C IV, Si IV, N V, C II, Si II} observable down to below 10^-2 solar abundance {4 mAngstrom EW limit}. This sightline is one of two prime FUSE targets for long-duration exposures in the extragalactic D/H program. FUSE will detect higher Ly-series lines and the Lyman break {accurate H I column density} and measure key metal lines {C III Lambda977, O VI Lambda1032, 1038}. Thus, the FUSE and STIS programs are highly interdependent.

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