An Aromatic Feature Emission Inventory of the Local Volume

Statistics – Methodology

Scientific paper

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Scientific paper

Using infrared photometry from the Spitzer Space Telescope, we perform the first inventory of aromatic feature emission for a large unbiased sample of galaxies in the local volume. The photometric methodology involved is calibrated and demonstrated to recover the aromatic fraction of the IRAC 8 micron flux with a standard deviation of 6% using a training set of 40 SINGS galaxies for which both equivalent photometry and suitable mid-infrared Spitzer IRS spectra were available. The resulting technique is then applied to the 258 galaxies from the Local Volume Legacy (LVL) survey, a large sample dominated by low-luminosity dwarf galaxies for which obtaining comparable MIR spectroscopy is not feasible. We find the total LVL luminosity due to five strong aromatic features in the 8 micron complex to be 2.47E10 solar luminosities with a mean volume density of 8.8E6 solar luminosities per cubic Mpc. Correspondingly, the same values for all mid-infrared aromatic features in the wavelength range 5.5-20 microns are approximately 1.9 times larger. Using oxygen abundances compiled from the literature, we report a correlation between aromatic feature strength and metallicity, albeit one with significant scatter.

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