activity
20072026
most citedHerschel Survey of Galactic OH+, H2O+, and H3O+: Probing the Molecular Hydrogen Fraction and Cosmic-Ray Ionization Rate

272 citations · 3.7k across the 56 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

51 papers · 1 filter

astro-ph.GA2026★ 1 cited

JWST imaging of the Pleiades: anisotropy of turbulence in the cold neutral medium

G. Vigoureux, N. Flagey, F. Boulanger +14

Interstellar medium studies rely on magnetohydrodynamic (MHD) turbulence as a framework for interpretation. In this context, the statistical characterization of interstellar observ…

astro-ph.GA2023★ 41 cited

Shock excitation of H in the James Webb Space Telescope era

L. E. Kristensen, B. Godard, P. Guillard +2

(Abridged) H2 is the most abundant molecule in the Universe. Thanks to its widely spaced energy levels, it predominantly lights up in warm gas, T > 100 K, such as shocked regions,…

astro-ph.GA2022★ 7 cited

HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules II. The absorption line survey with the IRAM 30 m telescope

W. -J. Kim, P. Schilke, D. A. Neufeld +11

As a complement to the HyGAL Stratospheric Observatory for Infrared Astronomy Legacy Program, we report the results of a ground-based absorption line survey of simple molecules in…

astro-ph.GA2022

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.…

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…

astro-ph.GA2022★ 40 cited

Gas condensation in Brightest Group Galaxies unveiled with MUSE

V. Olivares, P. Salome, S. L. Hamer +18

The origin of the cold gas in central galaxies in groups is still a matter of debate. We present Multi-Unit Spectroscopic Explorer (MUSE) observations of 18 optically selected loca…