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Primeval QSOsThe physical processes causing the formation of an increased number of QSOs at redshifts higher than 2 are discussed, along with the implications for the turn-on of active galactic nuclei (AGN) at the same time as QSOs. It is argued that optical and X-ray background data indicate that all but the brightest objects will decline in number at redshifts exceeding 2. Consideration is given to the possibility that accreting black holes are at the center of AGNs and formed within a few billion years of the turn-on of QSOs. A scenario is also explored wherein QSOs are remnant echoes of the epoch of galaxy formation and are thereby a suitable object with which to probe the parent population.
Document ID
19870040359
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Cavaliere, A.
(Roma II, Universita Rome, Italy)
Szalay, A. S.
(NASAFermilab Astrophysics Group, Batavia, IL; Eotvos Lorand Tudomanyegyetem Budapest, Hungary)
Date Acquired
August 13, 2013
Publication Date
December 15, 1986
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 311
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
87A27633
Distribution Limits
Public
Copyright
Other

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