The ice-surface reaction of C atoms with N2 is the dominant source of NH2CN and HNCNH in protostellar environments and dense clouds.
NH + H2CN → NH2 + HCN → H2CNNH → H2CNN + H → HCNNH + H → CH2 + N2 + H -273 -265 -116 0 +2 0.5 0.5 0 0 0 0 0 H2CNNH is likely produced but is not considered in the network
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The Reaction between Atomic Carbon and Molecular Nitrogen as a Source of Cyanamide and Carbodiimide on Interstellar Ices
The ice-surface reaction of C atoms with N2 is the dominant source of NH2CN and HNCNH in protostellar environments and dense clouds.