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20242026
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Showing 2025Show all

9 papers · 1 filter

astro-ph.GA2025

Weak, extended water vapor emission in the Horsehead nebula

Dariusz C. Lis, Vincent Maillard, Emeric Bron +4

We analyzed archival Herschel observations of water vapor emission toward the Horsehead photon dominated region (PDR), along with supporting ground-based and airborne observations…

astro-ph.GA2025

Interstellar medium phases and abundances in the central parsec: A JWST MIRI/MRS view of the Galactic center

P. Vermot, A. Ciurlo, D. Rouan +8

We used newly obtained observations from the Mid-Infrared Instrument (MIRI) equipped with the Medium Resolution Spectrometer (MRS) aboard the James Webb Space Telescope (JWST) to e…

astro-ph.GA2025

A Tentative Detection of Molecular Hydrogen (H) Emission Lines at Cosmic Dawn

Madisen Johnson, Blakesley Burkhart, Francesco D'Eugenio +11

We present a theoretical framework for interpreting far-ultraviolet (FUV) fluorescent emission from molecular hydrogen (H) in high-redshift galaxies, motivated by the unique ca…

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.GA2025

Estimating the dense gas mass of molecular clouds using spatially unresolved 3 mm line observations

Antoine Zakardjian, Annie Hughes, Jérôme Pety +28

We aim to develop a new method to infer the sub-beam probability density function (PDF) of H2 column densities and the dense gas mass within molecular clouds using spatially unreso…

astro-ph.GA2025

Tracers of the ionization fraction in dense and translucent molecular gas: II. Using mm observations to constrain ionization fraction across Orion B

Ivana Bešlić, Maryvonne Gerin, Viviana V. Guzmán +28

The ionization fraction () is a crucial parameter of interstellar gas, yet estimating it requires deep knowledge of molecular gas chemistry…