collaborators

6 papers

astro-ph.GA2025

PDRs4All XVII: Formation and excitation of HD in photodissociation regions. Application to the Orion Bar

Marion Zannese, Jacques Le Bourlot, Evelyne Roueff +12

The James Webb Space Telescope enabled the first detection of several rovibrational emission lines of HD in the Orion Bar, a prototypical photodissociation region. This provides an…

astro-ph.EP2025

Observation of an Accreting Planetary-Mass Companion with Signs of Disk-Disk Interaction in Orion

Emilie Vila, Paul Amiot, Olivier Berné +11

Young ( Myr) planetary-mass companions (PMCs) provide valuable insights into the formation and early evolution of planetary systems. To date, only a dozen such objects…

astro-ph.GA2025

Solar C/O ratio in planet-forming gas at 1 au in a highly irradiated disk

Ilane Schroetter, Olivier Berné, Emeric Bron +18

The chemical composition of exoplanets is thought to be influenced by the composition of the disks in which they form. JWST observations have unveiled a variety of species in numer…

astro-ph.GA2025

PDRs4All XI. Detection of infrared CH and CH rovibrational emission in the Orion Bar and disk d203-506: evidence of chemical pumping

Marion Zannese, Benoît Tabone, Emilie Habart +20

The methylidyne cation (CH) and the methyl cation (CH) are building blocks of organic molecules, yet their coupled formation and excitation mechanisms remain mainly unpro…

astro-ph.GA2024

A sensitivity analysis of the modeling of Polycyclic Aromatic Hydrocarbon emission in galaxies

Alexandros Maragkoudakis, Christiaan Boersma, Pasquale Temi +5

We have conducted a sensitivity analysis on the mid-infrared spectral decomposition of galaxies and the modeling of the PAH emission spectrum with the NASA Ames PAH Infrared Spectr…

astro-ph.GA2024

PDRs4All XIII. Empirical prescriptions for the interpretation of JWST imaging observations of star-forming regions

Ryan Chown, Yoko Okada, Els Peeters +17

(Abridged) JWST continues to deliver incredibly detailed infrared (IR) images of star forming regions in the Milky Way and beyond. IR emission from star-forming regions is very spe…