activity
20022021
most citedThe anatomy of the Orion B Giant Molecular Cloud: A local template for studies of nearby galaxies

206 citations · 1.1k across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.GA2021

Comparing absorption from classic tracers of the diffuse interstellar medium at optical and radio wavelengths along the same sightlines

Harvey Liszt

% aims To compare information gained from radio and optical absorption line profiles from the diffuse interstellar medium along the same sightline % methods We compare new and exis…

astro-ph.GA2021★ 11 cited

CO+ as a probe of the origin of CO in diffuse interstellar clouds

Maryvonne Gerin, Harvey Liszt

The chemistry of the diffuse interstellar medium is driven by the combined influences of cosmic rays, ultraviolet (UV) radiation, and turbulence. Previously detected at the outer e…

astro-ph.GA2020★ 8 cited

Reconciling X-ray and 21cm HI absorption gas column densities toward obscured AGN

Harvey Liszt

Hydrogen column densities inferred from X-ray absorption are typically 5 - 30 times larger than the neutral atomic hydrogen column densities derived from 21cm HI absorption toward…

astro-ph.GA2020★ 20 cited

Quantitative inference of the column densities from 3 mm molecular emission: A case study towards Orion B

Pierre Gratier, Jérôme Pety, Emeric Bron +21

Molecular hydrogen being unobservable in cold molecular clouds, the column density measurements of molecular gas currently rely either on dust emission observation in the far-IR or…

astro-ph.GA2020★ 25 cited

Tracers of the ionization fraction in dense and translucent gas: I. Automated exploitation of massive astrochemical model grids

Emeric Bron, Evelyne Roueff, Maryvonne Gerin +21

The ionization fraction plays a key role in the physics and chemistry of the neutral interstellar medium, from controlling the coupling of the gas to the magnetic field to allowing…

astro-ph.GA2020★ 8 cited

CO emission and CO hotspots in diffuse molecular gas

Harvey S Liszt

We observed 3mm \cotw, \coth, \coei, \hcop, HCN and CS emission from diffuse molecular gas along sightlines with \EBV\ 0.1 - 1 mag. Directions were mostly chosen for t…