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Evolution of Lyman-limit absorption systems over the redshift range 0.40 < Z < 4.69

Storrie-Lombardi, L. J. and McMahon, R. G. and Irwin, M. J. and Hazard, C. (1994) Evolution of Lyman-limit absorption systems over the redshift range 0.40 < Z < 4.69. Astrophysical Journal, 427 . L13-L16. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20170321-150231543

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Abstract

We present the results of a study of 15 z > 4.2 QSOs that extend statistical studies of Lyman-limit absorption line systems [N(H I) ≥ 1.6 x 10^(17) cm^(- 2)] to the highest redshifts currently possible. This data set has been combined with homogeneous data sets of low-redshift Hubble Space Telescope observations and intermediate-redshift ground-based observations. Assuming a power law of the form N(z) = N 0(1 + z)^γ for the number density, we find γ = 1.55 and N_0 = 0.27, with N = 3.27 per unit redshift at z = 4. The >99.7% confidence limits for y are 2.37 and 0.82. For the first time this indicates intrinsic evolution of these absorbers for an Q = 1 universe (γ = 1/2 for no evolution). This result is marginally consistent with no evolution for n = 0 (γ = 1 for no evolution). These results differ significantly from those of Sargent, Steidel, & Boksenberg (1989) who found no intrinsic evolution in Lyman-limit systems up to z = 3.5, and Lanzetta (1991) who found much stronger evolution for z > 2.5. For z ≾ 2 the space density of Lyman limit systems [N(1.5) ≈ 1.1] and Mg II absorbers with rest equivalent width W_0 > 0.3 Å [N(1.5) ≈ 1.0] is almost identical. This supports the picture that Lyman-limit and Mg II absorbers are drawn from the same population.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/187353DOIArticle
http://adsabs.harvard.edu/abs/1994ApJ...427L..13SADSArticle
ORCID:
AuthorORCID
Storrie-Lombardi, L. J.0000-0002-5987-5210
Additional Information:© 1994 American Astronomical Society. Received 1993 October 28; accepted 1994 March 4. We would like to thank Max Pettini and the referee for helpful suggestions. L. S. L. acknowledges support from an Isaac Newton Studentship and the Cambridge Overseas Trust. R. G. M. acknowledges the support of the Royal Society.
Funders:
Funding AgencyGrant Number
Isaac Newton StudentshipUNSPECIFIED
Cambridge Overseas TrustUNSPECIFIED
Royal SocietyUNSPECIFIED
Subject Keywords:galaxies: evolution - quasars: absorption lines
Record Number:CaltechAUTHORS:20170321-150231543
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170321-150231543
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:75286
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:22 Mar 2017 14:27
Last Modified:03 Oct 2019 16:48

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