4.6 Article

Metallicity as a criterion to select H2-bearing damped Lyman-α systems

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ASTRONOMY & ASTROPHYSICS
卷 456, 期 3, 页码 L9-L12

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EDP SCIENCES S A
DOI: 10.1051/0004-6361:20065769

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galaxies : high-redshift; galaxies quasars : absorption lines; galaxies quasars : individual : Q2343+125 galaxies quasars : individual : Q2348-011

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Aims. We characterize the importance of metallicity on the presence of molecular hydrogen in damped Lyman-alpha (DLA) systems. Methods. We constructed a representative sample of 18 DLA/sub-DLA systems with log N(H I) > 19.5 at high redshift (z(abs) > 1.8) and with metallicities relative to solar [X/H] > -1.3 (with [X/H] = log N(X)/N(H)-log (X/H)(circle dot) and X either Zn, S or Si). We gathered data covering the expected wavelength range of redshifted H-2 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 z(abs) = 2.431 toward Q2343+125 and at z(abs) = 2.426 toward Q2348-011. Q2348-011, 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(H-2)/(2N(H-2) + N(H I)) > -4 is as large as 50% for [X/H] > -0.7, when it is only similar to 5% for [X/H] < -1.3 and similar to 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.

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