Zinc as a tracer of metallicity evolution of Damped Lyman alpha systems

Details Zinc as a tracer of metallicity evolution of Damped Lyman alpha systems Zinc as a tracer of metallicity evolution of Damped Lyman alpha systems

2000-05-29

arxiv.org/abs/astro-ph/0005555v1

Astronomy and Astrophysics

Astrophysics

To appear in Astrophysical Journal. 7 pages, 2 figures

Scientific paper

10.1086/317110

Zinc is a good indicator of metallicity in Damped Lyman alpha (DLA) systems because it is almost unaffected by dust depletion. However, the use of zinc as a tracer of metallicity evolution has been hampered by the difficulty of detecting the Zn II resonance lines at high redshift. The measurement of zinc abundance in a DLA system at z_abs > 3 obtained by means of the UVES spectrograph at the VLT prompted us to re-analyse the full sample of zinc abundances present in the literature to search for a metallicity-redshift relation in DLA systems. The study of the metallicities of individual systems shows evidence for an anti-correlation between [Zn/H] and redshift supported by different types of statistical tools. The zinc metallicity decreases by -0.3 +/- 0.1 dex per unit redshift interval in the range 0.5 <~ z_abs <~ 3.5. This rate is in good agreement with that found by Savaglio, Panagia & Stiavelli (2000) in their recent study of DLA abundances corrected for dust depletion. The present result does not require a knowledge of the dust depletion pattern(s) in DLA systems. On the other hand, the analysis of the column-density weighted metallicity of the sample, , does not show a clear evidence for redshift evolution, consistent with previous studies of zinc abundances. We propose that the apparent lack of evolution of is due to the combination of selection bias effects together with the extreme sensitivity of to low-number statistics.

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