37 citations · 46 across the 5 of their papers we have counts for
5 papers
Neon is an inhibitor of CO hydrogenation in pre-stellar core conditions
Basile Husquinet, Julie Vitorino, Olli Sipilä +2
Neon (Ne) is the fifth most abundant element in the Universe. Because it is chemically inert, it has never been considered in astrochemical models that studied molecular evolution.…
A fast machine learning tool to predict the composition of astronomical ices from infrared absorption spectra
Andrés Megías, Izaskun Jiménez-Serra, François Dulieu +6
Current observations taken by James Webb Space Telescope (JWST) allow us to observe the absorption features of icy mantles that cover interstellar dust grains, which are mainly com…
Binding energies of ethanol and ethylamine on interstellar water ices: synergy between theory and experiments
Jessica Perrero, Julie Vitorino, Emanuele Congiu +3
Experimental and computational chemistry are two disciplines to conduct research in Astrochemistry, providing essential reference data for both astronomical observations and modeli…
Experimental study of the binding energy of NH3 on different types of ice and its impact on the snow line of NH3 and H2O
S. Kakkenpara Suresh, F. Dulieu, J. Vitorino +1
N-bearing molecules (like N2H+ or NH3) are excellent tracers of high-density, low-temperature regions like dense cloud cores and could shed light into snowlines in protoplanetary d…
Ammonia snow-lines and ammonium salts desorption
F. Kruczkiewicz, J. Vitorino, E. Congiu +2
Context. The nitrogen reservoir in planetary systems is a long standing problem. Part of the N-bearing molecules is probably incorporated into the ice bulk during the cold phases o…