Metallicity as a criterion to select H2-bearing damped Lyman-αsystems

Petitjean, P. ; Ledoux, C. ; Noterdaeme, P. ; Srianand, R. (2006) Metallicity as a criterion to select H2-bearing damped Lyman-αsystems Astronomy and Astrophysics, 456 (3). L9-L12. ISSN 0004-6361

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Official URL: http://www.aanda.org/articles/aa/abs/2006/36/aa576...

Related URL: http://dx.doi.org/10.1051/0004-6361:20065769

Abstract

Aims: We characterize the importance of metallicity on the presence of molecular hydrogen in damped Lyman- α(DLA) systems. Methods.We constructed a representative sample of 18 DLA/sub-DLA systems with log N(H I) > 19.5 at high redshift ( zabs > 1.8) and with metallicities relative to solar [X/H] > -1.3 (with [X/H] = log N(X)/N(H)-log (X/H) ⊙ and X either Zn, S or Si). We gathered data covering the expected wavelength range of redshifted H2 absorption lines on all systems in the sample from either the literature (10 DLAs), the UVES-archive, or new VLT-UVES observations for four of them. The sample is large enough to allow us to discuss for the first time the importance of metallicity as a criterion for the presence of molecular hydrogen in the neutral phase at high-z. Results.From the new observations, we report two new detections of molecular hydrogen in the systems at zabs=2.431 toward Q 2343+125 and at zabs= 2.426 toward Q 2348-011. Q 2348-011, From a comparison of the H2 detection fraction in the high-metallicity sample with earlier results, we find that the fraction of DLA systems with log f = log 2N(H2)/(2N(H2) + N(H I)) > -4 is as large as 50% for [X/H] > -0.7, when it is only ∼5% for [X/H] < -1.3 and ∼ 15% in the overall sample (with -2.5 < [X/H] < -0.3). This demonstrates that the presence of molecular hydrogen at high redshift is strongly correlated with metallicity.

Item Type:Article
Source:Copyright of this article belongs to EDP Sciences.
Keywords:Galaxies: High-redshift; Galaxies Quasars: Absorption Lines; Galaxies Quasars: Individual: Q 2343+125; Galaxies Quasars: Individual: Q 2348-011
ID Code:55224
Deposited On:18 Aug 2011 08:06
Last Modified:18 May 2016 07:34

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