Primeval Galaxies and OSO Absorbers

Details Primeval Galaxies and OSO Absorbers Primeval Galaxies and OSO Absorbers

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aps..may..b402c&link_type=abstract

American Physical Society, APS/AAPT Joint Meeting, May 2-5, 1996, abstract #B4.02

Physics

Scientific paper

With the advent of the 10-meter telescopes, absorption lines of carbon, silicon and nitrogen are now detected from low column density systems in the forest of neutral hydrogen lines which are seen in quasars. These lines allow us to study the onset of structure in the intergalactic gas and to determine the evolution of the physical properties of the gas. Abundances in the forest clouds are very similar to those of stars in our galactic halo, and we speculate on how and when this enrichment took place.

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