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
37 Citations
Formation of Hydroxylamine in Low-Temperature Interstellar Model Ices.
  • 12
  • PDF
Solid-state formation of CO 2 via the H 2 CO + O reaction
  • 18
  • PDF
Efficient formation route of the prebiotic molecule formamide on interstellar dust grains
  • 14
  • Highly Influenced
  • PDF
Solid state chemistry of nitrogen oxides--part I: surface consumption of NO.
  • 18
  • PDF
...
1
2
3
4
...

References

SHOWING 1-10 OF 107 REFERENCES
Water formation by surface O3 hydrogenation.
  • 61
  • PDF
Water formation at low temperatures by surface O2 hydrogenation II: The reaction network.
  • 109
  • PDF
Formation of hydroxylamine (NH2OH) in electron-irradiated ammonia-water ices.
  • 38
  • PDF
...
1
2
3
4
5
...