Metals, depletion and dimming: decrypting dust

TL;DR

This study analyzes the relationship between metals, dust, and depletions in the interstellar medium using a large sample of gamma-ray burst and quasar absorbers, revealing correlations consistent with local group relations and estimating cosmic dust dimming effects.

Contribution

It provides the largest sample to date for testing metal-dust relations and introduces a method to estimate cosmic dust dimming across redshifts based on observed depletion patterns.

Findings

Extinction correlates with volatile element column density, consistent with local group dust-to-metals ratio.

Refractory elements show a similar but less significant relation, offset from local group values.

Cosmic dust dimming becomes significant at redshifts 3-5, affecting observations of distant objects.

Abstract

Dust plays a pivotal role in the chemical enrichment of the interstellar medium. In the era of mid/high resolution spectra and multi-band spectral energy distributions, testing extinctions against gas and dust-phase properties is becoming possible. In order to test relations between metals, dust and depletions, and comparing those to the Local Group (LG) relations, we build a sample of 93 gamma-ray bursts and quasar absorbers (the largest sample so far) which have extinction and elemental column density measurements available. We find that extinctions and total column density of the volatile elements (Zn, S) are correlated (with a best-fit of dust-to-metals (DTM) 4.05x10-22 mag cm2) and consistent with the LG DTM relation. The refractory elements (Fe, Si) follow a similar, but less significant, relation offset about 1 dex from the LG relation. On the assumption that depletion onto dust grains is the cause, we compute the total (gas+dust-phase) column density and find a remarkable agreement with the LG DTM relation: a best-fit of 4.91x10-22 mag cm2. We then use our results to compute the amount of 'intervening metal from unknown sources' in random sightlines out to redshifts of z=5. Those metals implicate the presence of dust and give rise to an average 'cosmic dust dimming' effect which we express as a function of redshift, CDD(z). The CDD is unimportant out to redshifts of about 3, but because it is cumulative it becomes significant at redshifts z=3-5. Our results in this paper are based on a minimum of assumptions and effectively relying on observations.