THE REDSHIFT EVOLUTION OF THE LY-ALPHA FOREST

We have analyzed the properties of low column density Ly alpha forest clouds (12.8 less than or equal to logN(HI)less than or equal to 16.0) toward 5 QSOs at different redshifts, using high signal-to-noise data from the HIRES spectrograph on the Keck I 10 m telescope. The results are used to study the evolution of these clouds in the interval 2.1<z <3.5. We find: (1) The differential density distribution of forest clo uds, f(N-HI), fits an empirical power law with a typical slope of -1.3 5-->-l.55 for clouds with N(HI)less than or equal to 10(14.3)cm(-2) an d changes extremely slowly with redshift over this N-HI range. (2) The deviation of f(N-HI) from this power-law distribution at higher colum n densities depends on redshift: for higher redshifts, the departure f rom a power-law distribution occurs at higher N-HI, which means that h igher column density clouds rapidly disappear with decreasing redshift . This may be consistent with an invariant shape for the different col umn density distributions, but with a shift to a lower column density normalization for systems at different redshifts driven by the overall expansion of the universe. (3) The linewidths of the forest clouds in crease as redshift decreases. (4) The correlation strength of the fore st clouds seems to increase as redshift decreases. We discuss these re sults in terms of the evolution of the IGM comparing the results to mo dels and analytic descriptions of the evolution of structure in the ga s. (C) 1997 American Astronomical Society.