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The Evolution of Neutral Gas in the Universe

dc.contributor.authorTurnshek, David
dc.contributor.authorRao, Sandhya
dc.contributor.authorMonier, Eric
dc.contributor.authorNestor, Daniel
dc.contributor.authorQuider, Anna
dc.date.accessioned2021-09-07T18:02:38Z
dc.date.available2021-09-07T18:02:38Z
dc.date.issued2006-01-01
dc.identifier.citationDavid Turnshek, Sandhya Rao, Eric Monier, Daniel Nestor and Anna Quider (2006). The Evolution of Neutral Gas in the Universe. Proceedings of the International Astronomical Union, 2, pp 440-440. Available on the publisher's site at http://journals.cambridge.org/abstract_S1743921306010611 .
dc.identifier.urihttp://hdl.handle.net/20.500.12648/2631
dc.descriptionCopyright 2007 Cambridge University Press
dc.description.abstractWe give references to some of our work on the properties and evolution of the neutral gas component of the Universe (see reference list). The bulk of the observed neutral gas has been detected by identifying intervening damped Ly? (DLA) quasar absorption-line systems with N(H) > 2 × 1020 atoms cm ?2. We also present some initial results from a program to identify DLA absorbers near redshift z = 0.5 using Hubble Space Telescope ACS prism spectra
dc.subjectQuasars
dc.subjectAbsorption Lines
dc.subjectGalaxies
dc.subjectEvolution
dc.titleThe Evolution of Neutral Gas in the Universe
dc.typearticle
dc.source.journaltitleProceedings of the International Astronomical Union
dc.source.volume2
refterms.dateFOA2021-09-07T18:02:38Z
dc.description.institutionSUNY Brockport
dc.source.peerreviewedTRUE
dc.source.statuspublished
dc.description.publicationtitlePhysics
dc.contributor.organizationCambridge University
dc.contributor.organizationThe College at Brockport
dc.contributor.organizationUniversity of Pittsburgh
dc.languate.isoen_US


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