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20012024
most citedA model for atomic and molecular interstellar gas: The Meudon PDR code

538 citations · 7.6k across the 116 of their papers we have counts for

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Showing astro-ph.GAShow all

77 papers · 1 filter

astro-ph.GA2024★ 90 cited

Formation of the Methyl Cation by Photochemistry in a Protoplanetary Disk

Olivier Berné, Marie-Aline Martin-Drumel, Ilane Schroetter +53

Forty years ago it was proposed that gas phase organic chemistry in the interstellar medium was initiated by the methyl cation CH3+, but hitherto it has not been observed outside t…

astro-ph.GA2023★ 19 cited

HCN emission from translucent gas and UV-illuminated cloud edges revealed by wide-field IRAM 30m maps of Orion B GMC: Revisiting its role as tracer of the dense gas reservoir for star formation

M. G. Santa-Maria, J. R. Goicoechea, J. Pety +28

We present 5 deg^2 (~250 pc^2) HCN, HNC, HCO+, and CO J=1-0 maps of the Orion B GMC, complemented with existing wide-field [CI] 492 GHz maps, as well as new pointed observations of…

astro-ph.GA2023★ 115 cited

PDRs4All IV. An embarrassment of riches: Aromatic infrared bands in the Orion Bar

Ryan Chown, Ameek Sidhu, Els Peeters +136

(Abridged) Mid-infrared observations of photodissociation regions (PDRs) are dominated by strong emission features called aromatic infrared bands (AIBs). The most prominent AIBs ar…

astro-ph.GA2023★ 17 cited

The extremely sharp transition between molecular and ionized gas in the Horsehead nebula

C. Hernández-Vera, V. V. Guzmán, J. R. Goicoechea +12

(Abridged) Massive stars can determine the evolution of molecular clouds with their strong ultraviolet (UV) radiation fields. Moreover, UV radiation is relevant in setting the ther…

astro-ph.GA2023★ 3 cited

Gas phase Elemental abundances in Molecular cloudS (GEMS) VIII. Unlocking the CS chemistry: the CH + S CS + H and C + S CS + C reactions

Carlos M. R. Rocha, Octavio Roncero, Niyazi Bulut +15

We revise the rates of reactions CH + S -> CS + H and C_2 + S -> CS + C, important CS formation routes in dark and diffuse warm gas. We performed ab initio calculations to characte…

astro-ph.GA2023

Understanding the temperatures of H3+ and H2 in diffuse interstellar sightlines

Jacques Le Bourlot, Evelyne Roueff, Franck Le Petit +3

The triatomic hydrogen ion H3+ is one of the most important species for the gas phase chemistry of the interstellar medium. Observations of H3+ are used to constrain important phys…