The Nature and Evolution of Absorption-Selected Galaxies

Simple item page
dc.creatorSteidel, C.
dc.date1995-09-19
dc.date.accessioned2026-07-07T02:20:12Z
dc.date.available2026-07-07T02:20:12Z
dc.descriptionWe present results of surveys for high redshift galaxies selected by their having produced detectable Mg~II and Lyman limit absorption in the spectra of background QSOs. We discuss the properties of the absorbing galaxies, the connection between galaxy properties and absorption line signatures, and how a combination of QSO absorption line and conventional faint galaxy techniques can be used to study field galaxy evolution to very large redshifts.
dc.description14 pages, uuencoded, compressed postscript (includes figures). Review talk given at the ESO Workshop on QSO Absorption Lines, November 1994
dc.identifierhttps://arxiv.org/abs/astro-ph/9509098
dc.identifierhttp://arxiv.org/abs/astro-ph/9509098
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10138
dc.subjectAstrophysics
dc.titleThe Nature and Evolution of Absorption-Selected Galaxies
dc.typetext

Files

Collections

arXiv