activity
19992026
most citedThe CO-to-H2 Conversion Factor

2.2k citations · 13.2k across the 102 of their papers we have counts for

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Showing 2022Show all

7 papers · 1 filter

astro-ph.IM2022★ 41 cited

The PhotoDissociation Region Toolbox: Software and Models for Astrophysical Analysis

Marc W. Pound, Mark G. Wolfire

The PhotoDissociation Region Toolbox provides comprehensive, easy-to-use, public software tools and models that enable an understanding of the interaction of the light of young, lu…

astro-ph.GA2022★ 17 cited

Experimental determination of the dissociative recombination rate coefficient for rotationally-cold CH and its implications for the diffuse cloud chemistry

Daniel Paul, Manfred Grieser, Florian Grussie +13

Observations of CH are used to trace the physical properties of diffuse clouds, but this requires an accurate understanding of the underlying CH chemistry. Until this work,…

astro-ph.GA2022★ 8 cited

SOFIA FEEDBACK survey: PDR diagnostics of stellar feedback in different regions of RCW 49

M. Tiwari, M. Wolfire, M. W. Pound +13

We quantified the effects of stellar feedback in RCW 49 by determining the physical conditions in different regions using the [CII] 158 m and [OI] 63 m observations from SOFI…

astro-ph.GA2022★ 22 cited

High angular resolution near-IR view of the Orion Bar revealed by Keck/NIRC2

Emilie Habart, Romane Le Gal, Carlos Alvarez +7

Nearby Photo-Dissociation Regions (PDRs), where the gas and dust are heated by the far UV-irradiation emitted from stars, are ideal templates to study the main stellar feedback pro…

astro-ph.GA2022★ 178 cited

Photodissociation and X-Ray Dominated Regions

Mark G. Wolfire, Livia Vallini, Mélanie Chevance

The radiation from stars and active galactic nuclei (AGN) creates photodissociation regions (PDRs) and X-ray dominated regions (XDRs), where the chemistry or heating are dominated…

astro-ph.GA2022★ 20 cited

HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules -- I. Survey description and a first look toward W3(OH), W3 IRS5 and NGC 7538 IRS1

A. M. Jacob, D. A. Neufeld, P. Schilke +22

The HyGAL SOFIA legacy program surveys six hydride molecules -- ArH+, OH+, H2O+, SH, OH, and CH -- and two atomic constituents -- C+ and O -- within the diffuse interstellar medium…