High-ionization emission line ratios from quasar broad line regions: metallicity or density?

TL;DR

This study challenges the assumption that high-ionization emission line ratios directly indicate metallicity in quasar broad line regions, showing instead that density and ionization conditions can explain observed variations.

Contribution

It demonstrates that variations in line ratios are due to physical conditions like density and ionization, not metallicity, and proposes a model with two kinematically distinct emission regions.

Findings

Line ratios do not vary with luminosity, black hole mass, or accretion rate.

Observed line ratio changes can be explained by gas with solar metallicity under varying physical conditions.

Quasar emission regions likely consist of high-density clouds and lower-density gas, affecting line ratios.

Abstract

The flux ratios of high-ionization lines are commonly assumed to indicate the metallicity of the broad emission line region in luminous quasars. When accounting for the variation in their kinematic profiles, we show that the NV/CIV, (SiIV+OIV])/CIV and NV/Lya line ratios do not vary as a function of the quasar continuum luminosity, black hole mass, or accretion rate. Using photoionization models from CLOUDY , we further show that the observed changes in these line ratios can be explained by emission from gas with solar abundances, if the physical conditions of the emitting gas are allowed to vary over a broad range of densities and ionizing fluxes. The diversity of broad line emission in quasar spectra can be explained by a model with emission from two kinematically distinct regions, where the line ratios suggest that these regions have either very different metallicity or density. Both simplicity and current galaxy evolution models suggest that near-solar abundances, with parts of the spectrum forming in high-density clouds, are more likely. Within this paradigm, objects with stronger outflow signatures show stronger emission from gas which is denser and located closer to the ionizing source, at radii consistent with simulations of line-driven disc-winds. Studies using broad-line ratios to infer chemical enrichment histories should consider changes in density and ionizing flux before estimating metallicities.