[astro-ph.GA] The formation and survival of complex organic molecules (COMs) in cold interstellar environments depends on their interactions with icy dust grain surfaces.
amorphous solid water
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.
Experimental Investigation Of O2 Diffusion And Entrapment In Interstellar Amorphous Solid Water (ASW)
Interstellar ices are mainly composed of amorphous solid water (ASW) containing small amounts of hypervolatiles, such as O2, whose diffusion-limited reactions play a key role in space chemistry. Although O2 […]
CO Desorption From Interstellar Icy Grains Induced By IR Excitation Of Superhydrogenated PAHs
Infrared (IR) radiation dominates dense, interstellar clouds, yet its effect on icy grains remains largely unexplored.
Binding Energies Of Small Interstellar Molecules On Neutral And Charged Amorphous Solid Water Surfaces
The interstellar medium (ISM) is all but empty. To date, more than 300 molecules have already been discovered. Because of the extremely low temperature, the gas-phase chemistry is dominated by […]
Chemical Pathways of SO2 With Hydrogen Atoms On Interstellar Ice Analogues
Sulfur dioxide (SO2) is a sulfur-containing molecule expected to exist as a solid in the interstellar medium (ISM). In this study, we performed laboratory experiments and computational analyses on the […]
