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

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Showing astro-ph.SRShow all

9 papers · 1 filter

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.SR2017★ 16 cited

SOFIA/GREAT Discovery of Terahertz Water Masers

David A. Neufeld, Gary J. Melnick, Michael J. Kaufman +6

We report the discovery of water maser emission at frequencies above 1 THz. Using the GREAT instrument on SOFIA, we have detected emission in the 1.296411 THz 8(27)-7(34) transitio…

astro-ph.SR2015★ 34 cited

Hydrogen isotope exchanges between water and methanol in interstellar ices

A. Faure, M. Faure, P. Theulé +2

The deuterium fractionation of gas-phase molecules in hot cores is believed to reflect the composition of interstellar ices. The deuteration of methanol is a major puzzle, however,…

astro-ph.SR2015★ 5 cited

A new nonlocal thermodynamical equilibrium radiative transfer method for cool stars

Julien Lambert, Eric Josselin, Nils Ryde +1

Context: The solution of the nonlocal thermodynamical equilibrium (non-LTE) radiative transfer equation usually relies on stationary iterative methods, which may falsely converge i…

astro-ph.SR2013★ 129 cited

Interstellar chemistry of nitrogen hydrides in dark clouds

Romane Le Gal, Pierre Hily-Blant, Alexandre Faure +3

The aim of the present work is to perform a comprehensive analysis of the interstellar chemistry of nitrogen, focussing on the gas-phase formation of the smallest polyatomic specie…

astro-ph.SR2013★ 122 cited

Rotational quenching of H2CO by molecular hydrogen: cross-sections, rates, pressure broadening

Laurent Wiesenfeld, Alexandre Faure

We compute the rotational quenching rates of the first 81 rotational levels of ortho- and para-H2CO in collision with ortho- and para-H2, for a temperature range of 10-300 K. We ma…