Circumstellar Dust, PAHs, and Stellar Populations in Early-Type Galaxies: Insights from GALEX and WISE

TL;DR

This study investigates the presence and characteristics of circumstellar dust and PAHs in early-type galaxies using GALEX and WISE data, revealing widespread dust, complex radiation fields, and evidence of shock processing affecting PAH ratios.

Contribution

It provides the first comprehensive analysis of circumstellar dust and PAH features in early-type galaxies, linking dust properties to stellar populations and shock processing effects.

Findings

Circumstellar dust is common in early-type galaxies.

PAH ratios are influenced by shock processing, not just radiation fields.

WISE W1 mass-to-light ratios support IMF variation findings.

Abstract

A majority of early-type galaxies contain interstellar dust, yet the origin of this dust, and why the dust sometimes exhibits unusual polycyclic aromatic hydrocarbon (PAH) ratios, remains a mystery. If the dust is internally produced, it likely originates from the large number of AGB stars associated with the old stellar population. We present GALEX and WISE elliptical aperture photometry of $\sim310$ early-type galaxies with Spitzer mid-infrared spectroscopy and/or ancillary data from ATLAS3D, to characterize their circumstellar dust and the shape of the radiation field that illuminates the interstellar PAHs. We find that circumstellar dust is ubiquitous in early-type galaxies, which indicates some tension between stellar population age estimates and models for circumstellar dust production in very old stellar populations. We also use dynamical masses from ATLAS3D to show that WISE W1 (3.4 $\mu$m) mass-to-light ratios are consistent with the initial mass function variation found by previous work. While the stellar population differences in early-type galaxies correspond to a range of radiation field shapes incident upon the diffuse dust, the ratio of the ionization-sensitive $7.7\mu$m to $11.3\mu$m PAH feature does not correlate with the shape of the radiation field, nor to variations with the size-sensitive $11.3\mu$m to $17\mu$m ratio. The $7.7\mu$m to $11.3\mu$m PAH ratio does tend to be smaller in galaxies with proportionally greater $H_2$ emission, which is evidence that processing of primarily smaller grains by shocks is responsible for the unusual ratios, rather than substantial differences in the overall PAH size or ionization distribution.