Polycyclic aromatic hydrocarbons in the dwarf galaxy IC 10

Abstract

Infrared observations from the Spitzer Space Telescope archive are used to study the dust component of the interstellar medium in the IC~10 irregular galaxy. Dust distribution in the galaxy is compared to the distributions of H$\alpha$ and [SII] emission, neutral hydrogen and CO clouds, and ionizing radiation sources. The distribution of polycyclic aromatic hydrocarbons (PAH) in the galaxy is shown to be highly non-uniform with the mass fraction of these particles in the total dust mass reaching 4%. PAHs tend to avoid bright HII regions and correlate well with atomic and molecular gas. This pattern suggests that PAHs form in the dense interstellar gas. We propose that the significant decrease of the PAH abundance at low metallicity is observed not only globally (at the level of entire galaxies), but also locally (at least, at the level of individual HII regions). We compare the distribution of the PAH mass fraction to the distribution of high-velocity features, that we have detected earlier in wings of H$\alpha$ and SII lines, over the entire available galaxy area. No conclusive evidence for shock destruction of PAHs in the IC~10 galaxy could be found.

Accepted for publication in Astronomy Reports

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• Evolution of dust and molecular hydrogen in the Magellanic System
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• Dust Evolution in the Dwarf Galaxy Holmberg II
• Polycyclic aromatic hydrocarbons destruction in star-forming regions across 42 nearby galaxies
• 3.3 μm PAH observations of the central kiloparsecs of Centaurus A
• The Dust Content and Radiation Fields of Sample of Galaxies in the ELAIS-N1 Field