Physical Conditions in Low Z Absorption Line Systems in Qsos: Cycle 4

Physics

Scientific paper

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Hst Proposal Id #5177 Quasars &Amp, Agn Quasar Absorption

Scientific paper

In PG 1630+377, we will use the HRS to measure lines of He I at 584A,
and we will use the FOS (in a different proposal) to measure associated
Ly-alpha and Ly-beta lines. The relative abundance of He I determined
this way should yield clues to the conditions in the Lyman-alpha forest
clouds and the IGM at high redshift.

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