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
Solid-state formation of CO 2 via the H 2 CO + O reaction
Solid state chemistry of nitrogen oxides--part I: surface consumption of NO.
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