Excitation properties of galaxies with the highest [OIII]/[OII] ratios: No evidence for massive escape of ionizing photons

TL;DR

This study investigates whether local high-excitation galaxies leak ionizing photons, finding no evidence for significant photon escape and supporting models where galaxies are mostly ionization-bounded.

Contribution

It provides a comprehensive observational analysis of high-excitation galaxies using multiple emission lines, challenging the idea that these galaxies significantly contribute to cosmic reionization.

Findings

No evidence for >10% escape fraction of ionizing photons.

Spectral energy distributions cannot fully explain observed emission lines.

Ionization-bounded models fit the data well.

Abstract

The possibility that star-forming galaxies may leak ionizing photons is at the heart of many present-day studies that investigate the reionization of the Universe. We test this hypothesis on local blue compact dwarf galaxies of very high excitation. We assembled a sample of such galaxies by examining the spectra from Data Releases 7 and 10 of the Sloan Digital Sky Survey. We argue that reliable conclusions cannot be based on strong lines alone, and adopt a strategy that includes important weak lines such as [OI] and the high-excitation HeII and [ArIV] lines. Our analysis is based on purely observational diagrams and on a comparison of photoionization models with well-chosen emission-line ratio diagrams. We show that spectral energy distributions from current stellar population synthesis models cannot account for all the observational constraints, which led us to mimick several scenarios that could explain the data. These include the additional presence of hard X-rays or of shocks. We find that only ionization-bounded models (or models with an escape fraction of ionizing photons lower than 10%) are able to simultaneously explain all the observational constraints.