activity
19952026
most citedHerschel Survey of Galactic OH+, H2O+, and H3O+: Probing the Molecular Hydrogen Fraction and Cosmic-Ray Ionization Rate

272 citations · 10.3k across the 218 of their papers we have counts for

collaborators
Showing 2019 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2019★ 24 cited

Chlorine-bearing molecules in molecular absorbers at intermediate redshifts

S. H. J. Wallstrom, S. Muller, E. Roueff +3

We use observations of chlorine-bearing species in molecular absorbers at intermediate redshifts to investigate chemical properties and Cl/Cl isotopic ratios in the a…

astro-ph.GA2019★ 57 cited

Abundances of sulphur molecules in the Horsehead nebula. First NS+ detection in a photodissociation region

P. Rivière-Marichalar, A. Fuente, J. R. Goicoechea +8

Aims. Our goal is to complete the inventory of S-bearing molecules and their abundances in the prototypical photodissociation region (PDR) the Horsehead nebula to gain insight into…

astro-ph.GA2019★ 22 cited

Standing in the shadow of dark gas: ALMA observations of absorption from dark CO in the molecular DNM of Chamaeleon

H. Liszt, M. Gerin, I. Grenier

% context We had detected J=1-0 HCO+ absorption in 12 directions lacking detected CO emission in the outskirts of the Chamaeleon complex and on 1 sightline with integrated CO emiss…

astro-ph.GA2019★ 1 cited

The Life Cycle of Dust

Sarah Sadavoy, Mikako Matsuura, Lee Armus +24

Dust offers a unique probe of the interstellar medium (ISM) across multiple size, density, and temperature scales. Dust is detected in outflows of evolved stars, star-forming molec…

astro-ph.GA2019★ 37 cited

A dynamically young, gravitationally stable network of filaments in Orion B

Jan H. Orkisz, Nicolas Peretto, Jérôme Pety +15

Filaments are a key step on the path that leads from molecular clouds to star formation. However, their characteristics are heavily debated, and the exact processes that lead to th…

astro-ph.GA2019

Stellar Feedback in the ISM Revealed by Wide-Field Far-Infrared Spectral-Imaging

Javier R. Goicoechea, Maryvonne Gerin, Emeric Bron

The radiative and mechanical interaction of stars with their environment drives the evolution of the ISM and of galaxies as a whole. The far-IR emission (lambda ~30 to 350 microns)…