Dust and elemental abundances in Damped Ly alpha absorbers

Abstract

The effects of the dust on the determination of elemental abundances in damped Ly alpha (DLA) absorbers are investigated. Relations between the observed abundances measured in the gas phase and the overall abundances (gas plus dust) are derived as a function of dust-to-gas ratio, metallicity, element-to-element abundance pattern, average extinction coefficient of dust grains, and chemical composition of dust grains. A method is presented for determining dust-to-gas ratios, dust-to-metals ratios, and dust-corrected relative abundances in DLA absorbers by assuming dust of Galactic type and constant abundance ratios between iron-peak elements. The method is applied to a sample of 17 DLA absorbers with available Zn, Cr and/or Fe measurements. The resulting dust-to-gas ratios are mostly distributed between 2% and 25% of the Galactic value, in good quantitative agreement with the results from reddening studies of QSOs with foreground DLA absorption. A correlation is found between dust-to-gas ratio and metallicity in DLA galaxies, with a typical dust-to-metals ratio of ~ 60% the Galactic value. The derived dust-to-metals ratios are then used to correct from the effects of dust the abundance ratios [Si/Fe], [S/Fe], [Ti/Fe], [Mn/Fe], [Ni/Fe] available for a sub-sample of 9 absorbers. The [alpha/Fe] ratios corrected from dust do not show the enhancement characteristic of metal-poor Galactic stars, but instead have essentially solar values, within +/- 0.2 dex. This suggests that the chemical history of DLA absorbers is different from that experienced by the Milky Way. Evidences that point to dwarf galaxies, rather than to spiral galaxies, as important contributors to the DLA phenomenon are summarized.

29 pages, 2 figures, to be published in the Astrophysical Journal, part1, 1998, Feb. 1st

References in corpus (6)

• On the Kinematics of the Damped Lyman Alpha Protogalaxies
• The Metallicity of High Redshift Galaxies: The Abundance of Zinc in 34 Damped Lyman Alpha Systems from z = 0.7 to 3.4
• Abundance Patterns of Heavy Elements in Damped Lyman-Alpha Galaxies
• Evidence for Rotation in the Galaxy at z=3.15 Responsible for a Damped Lyman-alpha Absorption System in the Spectrum of Q2233+1310
• UV Interstellar Absorption Lines towards the Starburst Dwarf Galaxy NGC 1705
• Dwarf Galaxies with Gentle Star Formation and the Counts of Galaxies in the Hubble Deep Field

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