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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 2023Show all

6 papers · 1 filter

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.EP2023

The edge-on protoplanetary disk HH 48 NE II. Modeling ices and silicates

J. A. Sturm, M. K. McClure, J. B. Bergner +11

The abundance and distribution of ice in protoplanetary disks (PPD) is critical to understand the linkage between the composition of circumstellar matter and the composition of exo…

astro-ph.EP2023★ 21 cited

The edge-on protoplanetary disk HH 48 NE I. Modeling the geometry and stellar parameters

J. A. Sturm, M. K. McClure, C. J. Law +11

Context. Observations of edge-on disks are an important tool for constraining general protoplanetary disk properties that cannot be determined in any other way. However, most radia…

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…