Christopher J. R. Clark

Growth of aromatic hydrocarbon dust particles in the extremely metal-poor galaxy Sextans A

The mid-infrared spectrum of star-forming, high-metallicity galaxies is dominated by emission features from aromatic and aliphatic bonds in small carbonaceous dust grains, often referred to as polycyclic aromatic hydrocarbons (PAHs). In metal-poor galaxies, the abundance of PAHs...