Hidróxeno molecular protonado (Galician Wikipedia)

Analysis of information sources in references of the Wikipedia article "Hidróxeno molecular protonado" in Galician language version.

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archive.org

Hogness, T. R.; Lunn, E. G. (1925). "The Ionization of Hydrogen by Electron Impact as Interpreted by Positive Ray Analysis". Physical Review 26 (1): 44–55. doi:10.1103/PhysRev.26.44.
Trafton, L. M.; et al. (1993). "Detection of H₃⁺ from Uranus". Astrophysical Journal 405: 761. doi:10.1086/172404.
Brittain, S. D.; et al. (2004). "Interstellar H₃⁺ Line Absorption toward LkHα 101". Astrophysical Journal 606: 911–916. doi:10.1086/383024.

archive.today

"Triatomic Hydrogen". Department of Molecular and Optical Physics, University of Freiburg, Germany. Arquivado dende o orixinal o 30 de xuño de 2012. Consultado o 12 de abril de 2014.

doi.org

dx.doi.org

Raynor, Susanne; Herschbach Dudley R. ACS, ed. "Electronic structure of Rydberg states of triatomic hydrogen, neon hydride, hydrogen fluoride (H2F), H3O, NH4 and CH5 molecules.". J. Phys. Chem., 1982, (en inglés) 86 ((18)): 3592–3598. doi:10.1021/j100215a020.
Thomson, J. J. (1913). "Rays of Positive Electricity". Proceedings of the Royal Society A 89 (607): 1–20. doi:10.1098/rspa.1913.0057.
Hogness, T. R.; Lunn, E. G. (1925). "The Ionization of Hydrogen by Electron Impact as Interpreted by Positive Ray Analysis". Physical Review 26 (1): 44–55. doi:10.1103/PhysRev.26.44.
Watson, W. D. (1973). "The Rate of Formation of Interstellar Molecules by Ion-Molecule Reactions". Astrophysical Journal 183 (2): L17. doi:10.1086/181242.
Herbst, E.; Klemperer, W. (1973). "The Formation and Depletion of Molecules in Dense Interstellar Clouds". Astrophysical Journal 185: 505. doi:10.1086/152436.
Oka, T. (1980). "Observation of the Infrared Spectrum of H₃⁺". Physical Review Letters 45: 531–534. doi:10.1103/PhysRevLett.45.531.
Drossart, P.; et al. (1989). "Detection of H₃⁺ on Jupiter". Nature 340 (6234): 539. doi:10.1038/340539a0.
Geballe, T. R.; et al. (1993). "Detection of H₃⁺ Infrared Emission Lines in Saturn". Astrophysical Journal 408 (2): L109. doi:10.1086/186843.
Trafton, L. M.; et al. (1993). "Detection of H₃⁺ from Uranus". Astrophysical Journal 405: 761. doi:10.1086/172404.
Geballe, T. R.; Oka, T. (1996). "Detection of H₃⁺ in Interstellar Space". Nature 384 (6607): 334–335. doi:10.1038/384334a0.
McCall, B. J.; et al. (1998). "Detection of H₃⁺ in the Diffuse Interstellar Meduim Toward Cygnus OB2 No. 12". Science 279 (5358): 1910–1913. doi:10.1126/science.279.5358.1910.
McCall, B. J.; et al. (2004). "Dissociative Recombination of Rotationally Cold H₃⁺". Physical Review A 70 (5): 052716. doi:10.1103/PhysRevA.70.052716.
Herbst, E. (2000). "The Astrochemistry of H₃⁺". Phil. Trans. R. Soc. Lond. A. 358 (1774): 2523–2534. doi:10.1098/rsta.2000.0665.
McCall, B. J.; et al. (1999). "Observations of H₃⁺ in Dense Molecular Clouds". Astrophysical Journal 522: 338–348. doi:10.1086/307637.
Brittain, S. D.; et al. (2004). "Interstellar H₃⁺ Line Absorption toward LkHα 101". Astrophysical Journal 606: 911–916. doi:10.1086/383024.
McCall, B. J.; et al. (2003). "An Enhanced Cosmic-ray Flux towards ζ Persei Inferred from a Laboratory Study of the H₃⁺-e^- Recombination Rate". Nature 422 (6931): 500. doi:10.1038/nature01498.
Oka, T. (2006). "Interstellar H₃⁺". PNAS 103 (33): 12235–12242. doi:10.1073/pnas.0601242103.

uni-freiburg.de

frhephysik.uni-freiburg.de

"Triatomic Hydrogen". Department of Molecular and Optical Physics, University of Freiburg, Germany. Arquivado dende o orixinal o 30 de xuño de 2012. Consultado o 12 de abril de 2014.