Neon and Argon optical emission lines in ionized gaseous nebulae: Implications and applications

TL;DR

This study analyzes optical emission lines of neon and argon in ionized nebulae to improve abundance measurements, develop new correction factors, and propose diagnostics for high-redshift galaxy metallicities.

Contribution

It introduces new ionization correction factors for Ne and Ar, studies their abundance ratios, and proposes a novel diagnostic method for high-redshift galaxy metallicity estimation.

Findings

Ne/O ratio remains constant across metallicities.

Evidence of negative radial gradients of Ar/O in some spiral galaxies.

A new diagnostic using [OII], [NeIII], and Hdelta lines for high-z metallicity.

Abstract

In this work we present a study of the strong optical collisional emission lines of Ne and Ar in an heterogeneous sample of ionized gaseous nebulae for which it is possible to derive directly the electron temperature and hence the chemical abundances of neon and argon. We calculate using a grid of photoionization models new ionization correction factors for these two elements and we study the behaviour of Ne/O and Ar/O abundance ratios with metallicity. We find a constant value for Ne/O, while there seems to be some evidence for the existence of negative radial gradients of Ar/O over the disks of some nearby spirals. We study the relation between the intensities of the emission lines of [NeIII] at 3869 \AA and [OIII] at 4959 \AA and 5007 \AA. This relation can be used in empirical calibrations and diagnostic ratios extending their applicability to bluer wavelengths and therefore to samples of objects at higher redshifts. Finally, we propose a new diagnostic using [OII], [NeIII] and Hdelta emission lines to derive metallicities for galaxies at high z.