activity
20052024
most citedAmmonium salts are a reservoir of nitrogen on a cometary nucleus and possibly on some asteroids

180 citations · 2.4k across the 54 of their papers we have counts for

collaborators
Showing 2018Show all

6 papers · 1 filter

astro-ph.GA2018★ 55 cited

The Dense Gas Fraction in Galactic Center Clouds

E. A. C. Mills, A. Ginsburg, K. Immer +5

We present an analysis of gas densities in the central R=300 parsecs of the Milky Way, focusing on three clouds: GCM-0.02-0.07 (the 50 km/s cloud), GCM-0.13-0.08 (the 20 km/s cloud…

astro-ph.GA2018★ 23 cited

Collisional Excitation and Weak Maser Action of Interstellar Methanimine

Alexandre Faure, François Lique, Anthony J. Remijan

The inelastic cross sections and rate coefficients for the rotational excitation of methanimine (CHNH) by cold H have been determined quantum mechanically based on a new hi…

astro-ph.GA2018★ 37 cited

Modelling the molecular composition and nuclear-spin chemistry of collapsing prestellar sources

P. Hily-Blant, A. Faure, C. Rist +2

We study the gravitational collapse of prestellar sources and the associated evolution of their chemical composition. We use the University of Grenoble Alpes Astrochemical Network…

astro-ph.GA2018★ 36 cited

Abundance of HCN and its C and N isotopologues in L1498

Victor S. Magalhaes, Pierre Hily-Blant, Alexandre Faure +2

The isotopic ratio of nitrogen in nearby protoplanetary disks, recently measured in CN and HCN, indicates that a fractionated reservoir of nitrogen is available at the stage of com…

astro-ph.SR2018★ 13 cited

Electron-impact excitation of diatomic hydride cations II: OH and SH

James R Hamilton, Alexandre Faure, Jonathan Tennyson

R-matrix calculations combined with the adiabatic-nuclei-rotation and Coulomb-Born approximations are used to compute electron-impact rotational rate coefficients for two open-shel…

astro-ph.IM2018★ 36 cited

An efficient statistical method to compute molecular collisional rate coefficients

Jérôme Loreau, François Lique, Alexandre Faure

Our knowledge about the "cold" Universe often relies on molecular spectra. A general property of such spectra is that the energy level populations are rarely at local thermodynamic…