activity
20242026
most citedPDRs4All VII. The 3.3 m aromatic infrared band as a tracer of physical properties of the ISM in galaxies

14 citations · 24 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

A Detailed Analysis of Intermediate-scale Structure in Optical Extinction Curves: Expanded Census and Two-family Classification

C. M. Gunasekera, M. Decleir, K. D. Gordon +4

The features of interstellar extinction curves serve as powerful diagnostics for interstellar dust, revealing information about its composition, size distribution, and the physical…

astro-ph.GA2025

JWST observations of photodissociation regions III. Dust modelling at the illuminated edge of the Horsehead PDR

M. Elyajouri, A. Abergel, N. Ysard +19

Carbonaceous nano-grains are a significant component of interstellar dust and dominate the mid-infrared emission of photodissociation regions (PDRs). We study the evolution of nano…

astro-ph.GA2025★ 10 cited

PDRs4All XVI. Tracing aromatic infrared band characteristics in photodissociation region spectra with PAHFIT in the JWST era

Dries Van De Putte, Els Peeters, Karl D. Gordon +13

Photodissociation regions (PDRs) exhibit emission between 3-20 um known as the Aromatic Infrared Bands (AIBs), originating from small carbonaceous species such as polycyclic aromat…

astro-ph.GA2025

The Resolved Structure of a Low Metallicity Photodissociation Region

Ilyse Y. Clark, Karin Sandstrom, Mark Wolfire +14

Photodissociation Regions (PDRs) are key to understanding the feedback processes that shape interstellar matter in galaxies. One important type of PDR is the interface between HII…

astro-ph.GA2024★ 14 cited

PDRs4All VII. The 3.3 m aromatic infrared band as a tracer of physical properties of the ISM in galaxies

Ilane Schroetter, Olivier Berné, Christine Joblin +9

Aromatic infrared bands (AIBs) are a set of broad emission bands at 3.3, 6.2, 7.7, 8.6, 11.2, and 12.7 m, seen in the infrared spectra of most galaxies. With JWST, the 3.3 m…