activity
20042022
most citedComplete Depletion in prestellar cores

242 citations · 1.1k across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.GA2022★ 26 cited

The ortho-to-para ratio of water in interstellar clouds

A. Faure, P. Hily-Blant, C. Rist +3

The nuclear-spin chemistry of interstellar water is investigated using the University of Grenoble Alpes Astrochemical Network (UGAN). This network includes reactions involving the…

astro-ph.GA2020★ 17 cited

Depletion and fractionation of nitrogen in collapsing cores

P. Hily-Blant, G. Pineau des Forêts, A. Faure +1

Measurements of the nitrogen isotopic ratio in Solar System comets show a constant value, ~140, which is three times lower than the protosolar ratio, a highly significant differenc…

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.GA2015★ 6 cited

Challenging shock models with SOFIA OH observations in the high-mass star-forming region Cepheus A

A. Gusdorf, R. Guesten, K. M. Menten +13

OH is a key molecule in H2O chemistry, a valuable tool for probing physical conditions, and an important contributor to the cooling of shock regions. OH participates in the re-dist…

astro-ph.GA2015

Hyperfine transitions of 13CN from pre-protostellar sources

David Flower, Pierre Hily-Blant

Recent quantum mechanical calculations of rate coefficients for collisional transfer of population between the hyperfine states of 13CN enable their population densities to be dete…

astro-ph.GA2014★ 42 cited

Shocks in dense clouds. IV. Effects of grain-grain processing on molecular line emission

S. Anderl, V. Guillet, G. Pineau des Forêts +1

Grain-grain processing has been shown to be an indispensable ingredient of shock modelling in high density environments. For densities higher than \sim10^5 cm-3, shattering becomes…