Efficient surface formation route of interstellar hydroxylamine through NO hydrogenation. I. The submonolayer regime on interstellar relevant substrates.

@article{Congiu2012EfficientSF,
  title={Efficient surface formation route of interstellar hydroxylamine through NO hydrogenation. I. The submonolayer regime on interstellar relevant substrates.},
  author={E. Congiu and H. Chaabouni and C. Laffon and P. Parent and S. Baouche and F. Dulieu},
  journal={The Journal of chemical physics},
  year={2012},
  volume={137 5},
  pages={
          054713
        }
}
Dust grains in the interstellar medium are known to serve as the first chemical laboratory where the rich inventory of interstellar molecules are synthesized. Here we present a study of the formation of hydroxylamine--NH(2)OH--via the non-energetic route NO + H (D) on crystalline H(2)O and amorphous silicate under conditions relevant to interstellar dense clouds. Formation of nitrous oxide (N(2)O) and water (H(2)O, D(2)O) is also observed and the reaction network is discussed. Hydroxylamine and… Expand
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Efficient surface formation route of interstellar hydroxylamine through NO hydrogenation. II. The multilayer regime in interstellar relevant ices.
Experimental and Theoretical Study of the Chemical Network of the Hydrogenation of NO on Interstellar Dust Grains
Simultaneous hydrogenation and UV-photolysis experiments of NO in CO-rich interstellar ice analogues; linking HNCO, OCN−, NH2CHO, and NH2OH
Low-temperature surface formation of NH3 and HNCO: hydrogenation of nitrogen atoms in CO-rich interstellar ice analogues
Formation of Hydroxylamine in Low-Temperature Interstellar Model Ices.
Water formation through O2 + D pathway on cold silicate and amorphous water ice surfaces of interstellar interest.
Hydrogenation of CO-bearing species on grains: unexpected chemical desorption of CO
Solid-state formation of CO 2 via the H 2 CO + O reaction
Efficient formation route of the prebiotic molecule formamide on interstellar dust grains
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