2002ApJ...571..693P -
Astrophys. J., 571, 693-711 (2002/June-1)
The UCSD HIRES/Keck I damped Lyα abundance Database.(1) III. An empirical study of photoionization in the damped Lyα system toward GB 1759+7539.
PROCHASKA J.X., HOWK J.C., O'MEARA J.M., TYTLER D., WOLFE A.M., KIRKMAN D., LUBIN D. and SUZUKI N.
Abstract (from CDS):
We investigate the ionization state of the damped Lyα system at z=2.62 toward GB 1759+7539 through an analysis of ionic ratios sensitive to photoionization: Ar0/S+, Fe++/Fe+, N+/N0, and Al++/Al+. Approximately half of the metals arise in a mostly neutral velocity component with H I/H>0.9, based on Fe++/Fe+<0.013. In contrast, the remaining half exhibit Fe++/Fe+~0.3, indicative of a partially ionized medium with H I/H~0.5. These conclusions are supported by the observed N+/N0, Al++/Al+, and Ar0/Si+ ratios. We assess ionization corrections for the observed column densities through photoionization models derived from the CLOUDY software package. In the neutral gas, the ionization corrections are negligible, except for Ar0. However, for the partially ionized gas, element abundance ratios differ from the ionic ratios by 0.1-0.3 dex for (Si+, S+, Ni+, Al+)/Fe+ ratios and more for (N0, Ar0)/Fe+. Independent of the shape of the photoionizing spectrum and assumptions of the number of ionization phases, these ionization corrections have minimal impact (≲0.1 dex) on the total metallicity inferred for this damped Lyα system. Measurements of the relative elemental abundances of the partially ionized gas, however, have a greater than ~0.15 dex uncertainty, which hides the effects of nucleosynthesis and differential dust depletion. We caution the reader that this damped system is unusual for a number of reasons (e.g., a very low Ar0/S+ ratio), and we believe its ionization properties are special but not unique. Nevertheless, it clearly shows the value of examining photoionization diagnostics such as Fe++/Fe+ in a larger sample of damped systems.
Abstract Copyright:
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Journal keyword(s):
Galaxies: Abundances - Galaxies: Evolution - Nuclear Reactions, Nucleosynthesis, Abundances - Galaxies: Quasars: Absorption Lines
Simbad objects:
3
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