69 citations · 76 across the 3 of their papers we have counts for
4 papers
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…
Structures and Properties of Known and Postulated Interstellar Cations
Lorenzo Tinacci, Stefano Pantaleone, Andrea Maranzana +3
Positive ions play a fundamental role in the interstellar chemistry, especially in cold environments where chemistry is believed to be mainly ion-driven. However, in contrast with…
H2 formation on interstellar grains and the fate of reaction energy
Stefano Pantaleone, Joan Enrique-Romero, Cecilia Ceccarelli +4
Molecular hydrogen is the most abundant molecular species in the Universe. While no doubts exist that it is mainly formed on the interstellar dust grain surfaces, many details of t…
Chemical desorption versus energy dissipation: insights from ab-initio molecular dynamics of HCO formation
Stefano Pantaleone, Joan Enrique-Romero, Cecilia Ceccarelli +3
Molecular clouds are the cold regions of the Milky Way where stars form. They are enriched by rather complex molecules. Many of these molecules are believed to be synthesized on th…