Elemental Abundances from Intrinsic QSO Emission and Absorption Lines
Abstract
Several studies have shown that the column densities inferred from broad absorption lines (BALs) require extremely high metallicities and phosphorus overabundances -- apparently in conflict with other abundance diagnostics. Here I use HST spectroscopy of the BALQSO PG 1254+047 to argue that the BALs abundance estimates are incorrect, because partial line-of-sight coverage of the continuum source(s) has led to gross underestimates of the line optical depths and column densities. I claim that the significant presence of PV 1118,1128 absorption in this and other BALQSOs identifies the saturated absorption-line spectrum. This interpretation implies that the total column densities are at least ten times larger than previous estimates, namely log N_H(cm-2) > 22. The outflowing BAL gas, at velocities from -15,000 to -27,000 km/s in PG 1254+047, is therefore a strong candidate for the X-ray absorber in BALQSOs. If this high-column density outflow is radiately accelerated, it must originate <0.1 pc from the QSO.
Keywords
Cite
@article{arxiv.astro-ph/9806101,
title = {Elemental Abundances from Intrinsic QSO Emission and Absorption Lines},
author = {F. Hamann},
journal= {arXiv preprint arXiv:astro-ph/9806101},
year = {2007}
}
Comments
7 pages LaTeX with 2 figs. embedded