127 citations · 309 across the 8 of their papers we have counts for
4 papers · 1 filter
Where does the energy go during the interstellar NH formation on water ice? A computational study
Stefano Ferrero, Stefano Pantaleone, Cecilia Ceccarelli +3
In the coldest (10--20 K) regions of the interstellar medium, the icy surfaces of interstellar grains serve as solid-state supports for chemical reactions. Among their plausible ro…
Binding Energies of Interstellar Relevant S-bearing Species on Water Ice Mantles: A Quantum Mechanical Investigation
J. Perrero, J. Enrique-Romero, S. Ferrero +5
Binding energies (BEs) are one of the most important parameters for astrochemical modeling determining, because they govern whether a species stays in the gas-phase or is frozen on…
Acetaldehyde binding energies: a coupled experimental and theoretical study
S. Ferrero, F. Grieco, A-S. Ibrahim Mohamed +6
Acetaldehyde is one of the most common and abundant gaseous interstellar complex organic molecules, found in cold and hot regions of the molecular interstellar medium. Its presence…
Theoretical distribution of the ammonia binding energy at interstellar icy grains: a new computational framework
Lorenzo Tinacci, Aurele Germain, Stefano Pantaleone +3
The binding energies (BE) of molecules on the interstellar grains are crucial in the chemical evolution of the interstellar medium (ISM). Both temperature programmed desorption (TP…