Quasar absorption line studies of galaxies and the intergalactic medium at z>1.5

Details Quasar absorption line studies of galaxies and the intergalactic medium at z>1.5 Quasar absorption line studies of galaxies and the intergalactic medium at z>1.5

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..470...79s&link_type=abstract

The 9th astrophysics conference: After the dark ages, when galaxies were young (the Universe at 2<Z<5). AIP Conference Proceedi

Astronomy and Astrophysics

Astrophysics

Intergalactic Matter, Quasar Absorption And Emission-Line Systems, Lyman Forest, Observational Cosmology

Scientific paper

The title of this article could of course encompass an entire meeting. I will focus my comments on reviewing of what we know about the most numerous absorption lines, the neutral hydrogen absorbers, and their evolution with redshift. This field of study has undergone a renaissance in last few years driven by observations with the Hubble Space Telescope of low redshift quasar absorption lines, observations of high redshift absorbers with the HIRES instrument on Keck, and cosmological modeling that allows us to make detailed comparisons of lines of sight through simulated universes.

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