2 papers
astro-ph.GA2026
Using astrochemical models to simulate reactivity experiments on cold surfaces
Valeriia Sokolova, Basile Husquinet, Stephan Diana +7
The development of molecular complexity during stellar and planetary formation owes much to the interaction of gas and dust. When the first astrochemical models including solid-sta…
astro-ph.GA2025
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.…