What it is
Polycyclic aromatic hydrocarbons (PAHs), small carbonaceous dust grains, dominate the mid-infrared spectra of star-forming, metal-rich galaxies, but their abundance relative to total dust drops sharply in metal-poor galaxies, and the origin of this deficit is unknown. With the James Webb Space Telescope the authors detected and resolved PAH emission in Sextans A, a galaxy with 7% of the Sun's metallicity and, to their knowledge, the lowest-metallicity PAH detection so far. The emission comes from compact clumps 3 to 10 parsecs across, which explains why lower-resolution instruments missed it, and the ratios of the 3.3, 7.7 and 11.3 micron features indicate small, neutral grains with no evidence of substantial processing by radiation.
Why it matters
The results favour inhibited grain growth over enhanced destruction as the origin of the low PAH abundance in Sextans A, with the compact clumps likely active sites of PAH growth within a dense, well-shielded phase of the interstellar medium. They show that PAHs can form and survive in the extremely metal-poor environments that were common early in the evolution of the Universe.
Every metric behind this entry is listed, with its source, under Sources and data below.
Filed underAstrophysics and Star Formation Studies, Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research