Ultraluminous Infrared Galaxies and the Origin of QSOs

Simple item page
dc.creatorSanders, D. B.
dc.date2001-09-09
dc.date.accessioned2026-07-07T01:59:53Z
dc.date.available2026-07-07T01:59:53Z
dc.descriptionWe review the evidence which suggests that ultraluminous infrared galaxies (ULIGs) are the precursors of optically selected quasi-stellar objects (QSOs) and discuss additional data that suggests that the majority, if not all QSOs, may begin their lives in an intense infrared phase. Implications for the host galaxies of QSOs are discussed.
dc.descriptionLaTex, 11 pages with 7 embedded postscript figures, Review presented at the Workshop on "QSO Hosts and Their Environments", Granada, Spain, 10-12 January, 2001
dc.identifierhttps://arxiv.org/abs/astro-ph/0109138
dc.identifierhttp://arxiv.org/abs/astro-ph/0109138
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3295
dc.subjectAstrophysics
dc.titleUltraluminous Infrared Galaxies and the Origin of QSOs
dc.typetext

Files

Collections

arXiv