Gas-phase formation of glycolonitrile in the interstellar medium
Luis Guerrero-Méndez, Anxo Lema-Saavedra, Elena Jiménez, Antonio Fernández‐Ramos, Emilio Martı́nez-Núñez
Abstract
within the 10-150 K temperature range. Our calculations indicate that the formation of both hydrogen isocyanide and glycolonitrile is efficient under the harsh conditions of the ISM.
Topics & Concepts
Interstellar mediumGas phaseAstrobiologyPhase (matter)PhysicsChemical physicsChemistryAstrophysicsThermodynamicsGalaxyQuantum mechanicsAtmospheric chemistry and aerosolsMolecular Spectroscopy and StructureAdvanced Chemical Physics Studies