9 research outputs found
The Lyman Alpha Forest in the Spectra of QSOs
Observations of redshifted Lyman alpha forest absorption in the spectra of
quasistellar objects (QSOs) provide a highly sensitive probe of the
distribution of gaseous matter in the universe. Over the past two decades
optical spectroscopy with large ground-based telescopes, and more recently
ultraviolet spectroscopy from space have yielded a wealth of information on
what appears to be a gaseous, photoionized intergalactic medium, partly
enriched by the products of stellar nucleosynthesis, residing in coherent
structures over many hundreds of kiloparsecs. Recent progress with cosmological
hydro-simulations based on hierarchical structure formation models has led to
important insights into the physical structures giving rise to the forest. If
these ideas are correct, a truely inter- and proto-galactic medium [at high
redshift (z ~ 3), the main repository of baryons] collapses under the influence
of dark matter gravity into flattened or filamentary structures, which are seen
in absorption against background QSOs. With decreasing redshift, galaxies
forming in the denser regions, may contribute an increasing part of the Lyman
alpha absorption cross-section. Comparisons between large data samples from the
new generation of telescopes and artificial Lyman alpha forest spectra from
cosmological simulations promise to become a useful cosmological tool.Comment: latex plus three postscript figures, uses psfig,sty; Annual Review of
Astronomy and Astrophysics 1998, vol. 36 (in press