Reactions occurring on the ice-covered surfaces of interstellar dust grains are considered to be among the most important sources of complex species in the interstellar medium. Despite this, molecules such […]
interstellar dust grain
Machine Learning Exploration Of Binding Energy Distributions Of H2O At Astrochemically Relevant Dust Grain Surfaces
Binding energies (BEs) of adsorbates on interstellar dust grains critically control adsorption, desorption, diffusion, and surface reactivity, and therefore strongly influence astrochemical models of star- and planet-forming regions.
Deuteration Of HC3N And CH3CCH In The Pre-stellar Core L1544
Deuterated molecules are a useful diagnostic tool to probe the evolution and the kinematics in the earliest stages of star formation.
CO Diffusion on Interstellar Amorphous Solid Water: A Computational Study
Surface chemistry on interstellar dust grains is recognized as a central component in astrochemical models, representing a plausible formation route for many of the observed complex molecular species.
Photochemistry Of Interstellar Ice Forming Complex Organic Molecules
Processes expected to play a role in interstellar ice are simulated in the laboratory. Energetic photons and ions lead to fragmentation or desorption of molecules from the ice. The end […]
