JWST Discovery of Warm Dust in the Circumgalactic Medium of the Makani Galaxy
Sylvain Veilleux, Steven D. Shockley, Marcio Melendez, David S. N. Rupke, Alison L. Coil, Aleksandar M. Diamond-Stanic, James E. Geach, Ryan C. Hickox, John Moustakas, Gregory H. Rudnick, Paul H. Sell, Christy A. Tremonti, and Hojoon Cha

TL;DR
This study uses JWST infrared observations to detect and analyze warm dust and PAHs in the circumgalactic medium of the Makani Galaxy, revealing dust survival and processing in galactic winds over hundreds of millions of years.
Contribution
First detection of PAHs in the CGM of a galaxy with a large-scale starburst wind, showing dust survival and evolution over long distances.
Findings
PAHs detected up to 35 kpc in the galaxy's halo.
PAH properties vary with distance, indicating changes in starlight and ionization.
Dust survives long journeys in galactic winds but undergoes erosion.
Abstract
We report the detection of near- and mid-infrared emission from polycyclic aromatic hydrocarbons (PAHs) out to ~ 35 kpc in the Makani Galaxy, a compact massive galaxy with a record-breaking 100-kpc scale starburst-driven wind at redshift z = 0.459. The NIRCam and MIRI observations with JWST take advantage of a coincidental match between the PAH spectral features at 3.3, 7.7, and (11.3 + 12.2) microns in Makani and the bandpasses of the MIRI and NIRCam filters. The warm dust is not only detected in the cool-gas tracers of the galactic wind associated with the more recent (7 Myr) starburst episode, but also in the outer warm-ionized gas wind produced by the older (0.4 Gyr) episode. The presence of PAHs in the outer wind indicates that the PAHs have survived the long (R/v ~ 10^8 yrs) journey to the halo despite the harsh environment of the galactic wind. The measured F1800W/F1130W flux…
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