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A Model of Metallicity Evolution in the Early Universe

Wasserburg, G. J. and Qian, Y.-Z. (2000) A Model of Metallicity Evolution in the Early Universe. Astrophysical Journal Letters, 538 (2). L99-L102. ISSN 2041-8205. https://resolver.caltech.edu/CaltechAUTHORS:20131119-095347998

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Abstract

We apply the phenomenological model used to explain the abundances of Fe and r-process elements in very metal-poor stars in the Galaxy to [Fe/H] of damped Lyα systems. It is assumed that the first stars that formed after the big bang were very massive and that they promptly enriched the interstellar medium to [Fe/H] ~ -3, at which metallicity the formation of normal stars took over. Subsequent Fe enrichment was provided by Type II supernovae. The range of [Fe/H] at a given redshift z for damped Lyα systems is explained by the time t* after the big bang at which normal star formation started in an individual protogalactic system. The average t* is ≈80% the age of the universe for damped Lyα systems at z ≈ 1.5-4.5, indicating a long delay between the big bang and the turn-on of protogalaxies. It is inferred that a substantial fraction of the total baryonic matter may not have been aggregated into protogalaxies with normal star formation events until a late time corresponding to z ~ 1.5. The data near z = 2.2 indicate that the rate of turn-on of protogalaxies was initially very low and that it slowly reached a maximum at ~3 Gyr after the big bang. This rate of turn-on of galaxies may be important in understanding the rate of formation of quasars.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/312812DOIArticle
http://iopscience.iop.org/1538-4357/538/2/L99PublisherArticle
http://arxiv.org/abs/astro-ph/0006082arXivDiscussion Paper
ORCID:
AuthorORCID
Wasserburg, G. J.0000-0002-7957-8029
Additional Information:© 2000 The American Astronomical Society. Received 2000 April 11; accepted 2000 June 5; published 2000 July 21. We want to thank Roger Blandford and Marc Kamionkowski for their ongoing interest in this work and for generously giving their time and providing, as usual, deep cosmic insights and education. Maarten Schmidt has been kind enough to expose us to the details of quasar distribution. This work was supported in part by the Department of Energy under grant DE-FG02-87ER40328 to Y.-Z. Q. and by NASA under grant NAG5-4083 to G. J. W., Caltech Division Contribution 8728(1059).
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)DE-FG02-87ER40328
NASANAG5-4083
Subject Keywords:galaxies: abundances; galaxies: evolution; quasars: absorption lines
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences8728
Lunatic Asylum Lab1059
Issue or Number:2
Record Number:CaltechAUTHORS:20131119-095347998
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20131119-095347998
Official Citation:A Model of Metallicity Evolution in the Early Universe G. J. Wasserburg and Y.-Z. Qian 2000 ApJ 538 L99
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:42557
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:20 Nov 2013 21:07
Last Modified:09 Mar 2020 13:19

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