JWST Discovery of Warm Dust in the Circumgalactic Medium of the Makani Galaxy

Fuente: arXiv
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Auteurs principaux: Veilleux, Sylvain, Shockley, Steven D., Melendez, Marcio, Rupke, David S. N., Coil, Alison L., Diamond-Stanic, Aleksandar M., Geach, James E., Hickox, Ryan C., Moustakas, John, Rudnick, Gregory H., Sell, Paul H., Tremonti, Christy A., Cha, Hojoon
Format: Preprint
Publié: 2025
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author Veilleux, Sylvain
Shockley, Steven D.
Melendez, Marcio
Rupke, David S. N.
Coil, Alison L.
Diamond-Stanic, Aleksandar M.
Geach, James E.
Hickox, Ryan C.
Moustakas, John
Rudnick, Gregory H.
Sell, Paul H.
Tremonti, Christy A.
Cha, Hojoon
author_facet Veilleux, Sylvain
Shockley, Steven D.
Melendez, Marcio
Rupke, David S. N.
Coil, Alison L.
Diamond-Stanic, Aleksandar M.
Geach, James E.
Hickox, Ryan C.
Moustakas, John
Rudnick, Gregory H.
Sell, Paul H.
Tremonti, Christy A.
Cha, Hojoon
contents 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 ratios in the unresolved nucleus, inner halo (R = 10 - 20 kpc), and outer halo (R = 20 - 35 kpc), tracers of the PAH (11.3 + 12.2)/7.7 ratios, indicate decreasing starlight intensity incident on the PAHs, decreasing PAH sizes, and increasing PAH ionization fractions with increasing distance from the nucleus. These data provide the strongest evidence to date that the ejected dust of galactic winds survives the long journey to the CGM, but is eroded along the way.
format Preprint
id arxiv_https___arxiv_org_abs_2507_08098
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle JWST Discovery of Warm Dust in the Circumgalactic Medium of the Makani Galaxy
Veilleux, Sylvain
Shockley, Steven D.
Melendez, Marcio
Rupke, David S. N.
Coil, Alison L.
Diamond-Stanic, Aleksandar M.
Geach, James E.
Hickox, Ryan C.
Moustakas, John
Rudnick, Gregory H.
Sell, Paul H.
Tremonti, Christy A.
Cha, Hojoon
Astrophysics of Galaxies
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 ratios in the unresolved nucleus, inner halo (R = 10 - 20 kpc), and outer halo (R = 20 - 35 kpc), tracers of the PAH (11.3 + 12.2)/7.7 ratios, indicate decreasing starlight intensity incident on the PAHs, decreasing PAH sizes, and increasing PAH ionization fractions with increasing distance from the nucleus. These data provide the strongest evidence to date that the ejected dust of galactic winds survives the long journey to the CGM, but is eroded along the way.
title JWST Discovery of Warm Dust in the Circumgalactic Medium of the Makani Galaxy
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2507.08098