1998/08/31 by Scott F. Anderson, Craig J. Hogan, Benjamin F. Williams +2 · 1 citation
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #astro-ph
paper · pdf · doi:10.1086/300698
published as Astron.J.117:56-62,1999 · 17 pages including 5 figures. As accepted for publication in The Astronomical Journal (minor revisions)
arxiv created 1998/09/18 · openalex publication_date 1999/01/01 · arxiv updated 2009/12/01 · openalex created_date 2017/03/16 · openalex updated_date 2026/07/31
We present a new HST /STIS spectrum of the z = 3.18 quasar PKS 1935-692 and summarize the spectral features shortward of 304 Å in the rest frame likely to be caused by foreground He II Lyα absorption. In accord with the previous results on two other quasars at similar redshifts, we demonstrate a correlation with the H I Lyα forest absorption and show that much of the helium absorption is caused by a comparable quantity of more diffuse gas with Ω g ∼ 10 -2 , which is not detected in H I. The helium ionization zone around the quasar is detected, and a void is seen in both H I and He II. The properties of the absorption are in broad agreement with those of the other quasars and with models of the protogalactic gas distribution and ionization at this redshift.