92 citations · 527 across the 20 of their papers we have counts for
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3D chemical structure of the diffuse turbulent ISM II -- Origin of CH, new solution to an 80 years mystery
Benjamin Godard, Guillaume Pineau Des Forêts, Patrick Hennebelle +2
Aims: The large abundances of CH in the diffuse interstellar medium (ISM) are a long standing issue of our understanding of the thermodynamical and chemical states of the gas.…
Is the mm/submm dust polarization a robust tracer of the magnetic field topology in protostellar envelopes? A model exploration
Valeska Valdivia, Anaëlle Maury, Patrick Hennebelle
High resolution (sub-)millimeter polarization observations have opened a new era in the understanding of how B-fields are organized in star forming regions, unveiling an intricate…
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…