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20002026
most citedAn Ice Age JWST inventory of dense molecular cloud ices

363 citations · 2.7k across the 52 of their papers we have counts for

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Showing astro-ph.GAShow all

29 papers · 1 filter

astro-ph.GA2026

H2 emission in the Orion Bar, NGC7023 and the Horsehead Nebula observed with the James Webb Space Telescope

M. Zannese, A. Sidhu, A. Guerras +25

Molecular hydrogen (H2), the most abundant molecule in the interstellar medium, is a handy tool to study Photodissociation Regions. The JWST, with its high spatial resolution, sens…

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★ 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★ 16 cited

Astrochemical models of interstellar ices: History matters

A. Clément, A. Taillard, V. Wakelam +6

Ice is ubiquitous in the interstellar medium. We model the formation of the main constituents of interstellar ices, including H2O, CO2 , CO, and CH3 OH. We strive to understand wha…

astro-ph.GA2023★ 363 cited

An Ice Age JWST inventory of dense molecular cloud ices

M. K. McClure, W. R. M. Rocha, K. M. Pontoppidan +39

Icy grain mantles are the main reservoir of the volatile elements that link chemical processes in dark, interstellar clouds with the formation of planets and composition of their a…

astro-ph.GA2023★ 7 cited

Constraints on the non-thermal desorption of methanol in the cold core LDN 429-C

A. Taillard, V. WakelaM, P. Gratier +6

Cold cores are an early step of star formation, characterized by densities > 10 cm, low temperatures (< 15 K), and very low external UV radiation. We investigate the phy…