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arXiv.org e-Print Archive
Preprint . 2001
Data sources: arXiv.org e-Print Archive
https://dx.doi.org/10.48550/ar...
Article . 2001
License: arXiv Non-Exclusive Distribution
Data sources: Datacite
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Ultraluminous Infrared Galaxies and the Origin of QSOs

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Jan 2001Embargo end date: 01 Jan 2001Publisher:arXiv
Authors: Sanders, D. B.;

doi: 10.48550/arxiv.astro-ph/0109138

arXiv: http://arxiv.org/abs/astro-ph/0109138

Ultraluminous Infrared Galaxies and the Origin of QSOs

Abstract

We 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.

LaTex, 11 pages with 7 embedded postscript figures, Review presented at the Workshop on "QSO Hosts and Their Environments", Granada, Spain, 10-12 January, 2001

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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