Binding energies of interstellar molecules on crystalline and amorphous models of water ice by ab initio calculations

S Ferrero, L Zamirri, C Ceccarelli, A Witzel… - The Astrophysical …, 2020 - iopscience.iop.org
In the denser and colder (≤ 20 K) regions of the interstellar medium (ISM), near-infrared
observations have revealed the presence of submicron-sized dust grains covered by several …

Binding energies of interstellar relevant S-bearing species on water ice mantles: a quantum mechanical investigation

J Perrero, J Enrique-Romero, S Ferrero… - The Astrophysical …, 2022 - iopscience.iop.org
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 …

Binding Energies of N-bearing Species on Interstellar Water Ice Mantles by Quantum Chemical Calculations

B Martínez-Bachs, S Ferrero, C Ceccarelli… - The Astrophysical …, 2024 - iopscience.iop.org
Of the about 300 gas-phase molecular species so far detected in the interstellar medium
(ISM), mostly via observations of their rotational lines, around 40% contain nitrogen (N) …

[HTML][HTML] Adsorption of HCN on cosmic silicates: a periodic quantum mechanical study

N Bancone, S Pantaleone, P Ugliengo… - Physical Chemistry …, 2023 - pubs.rsc.org
Hydrogen cyanide (HCN) represents a small but widely distributed fraction of the interstellar
molecules, and it has been observed in all the environments characterizing the formation of …

Descriptors for binding energies at clusters: The case of nanosilicates as models of interstellar dust grains

M Andersen, AM Slavensky - The Journal of Chemical Physics, 2023 - pubs.aip.org
Binding energies of radicals and molecules at dust grain surfaces are important parameters
for understanding and modeling the chemical inventory of interstellar gas clouds. While first …

[PDF][PDF] Adsorption of HCN on cosmic silicates: a periodic quantum mechanical study1

M Corno - Phys. Chem. Chem. Phys, 2023 - academia.edu
Hydrogen cyanide (HCN) represents a small but widely distributed fraction of the interstellar
molecules, and it has been observed in all the environments characterizing the formation of …