Tham khảo Heli hydride cation

  1. ↑ “hydridohelium(1+) (CHEBI:33688)”. Chemical Entities of Biological Interest (ChEBI). European Bioinformatics Institute.
  2. 1 2 “Hydridohelium (CHEBI:33689)”. Chemical Entities of Biological Interest (ChEBI). European Bioinformatics Institute.
  3. 1 2 3 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. Bibcode:1925PhRv...26...44H. doi:10.1103/PhysRev.26.44.
  4. ↑ Coxon, J.; Hajigeorgiou, P. G. (1999). “Experimental Born–Oppenheimer Potential for the X1Σ+ Ground State of HeH+: Comparison with the Ab Initio Potential”. Journal of Molecular Spectroscopy. 193 (2): 306–318. Bibcode:1999JMoSp.193..306C. doi:10.1006/jmsp.1998.7740. PMID 9920707.
  5. ↑ Dias, A. M. (1999). “Dipole Moment Calculation to Small Diatomic Molecules: Implementation on a Two-Electron Self-Consistent-Field ab initio Program” (PDF). Rev da Univ de Alfenas. 5 (1): 77–79. Bản gốc (PDF) lưu trữ ngày 19 tháng 4 năm 2019. Truy cập ngày 22 tháng 4 năm 2019.
  6. ↑ Engel, Elodie A.; Doss, Natasha; Harris, Gregory J.; Tennyson, Jonathan (2005). “Calculated spectra for HeH+ and its effect on the opacity of cool metal-poor stars”. Monthly Notices of the Royal Astronomical Society. 357 (2): 471–477. arXiv:astro-ph/0411267. Bibcode:2005MNRAS.357..471E. doi:10.1111/j.1365-2966.2005.08611.x.
  7. ↑ Coyne, John P.; Ball, David W. (2009). “Alpha particle chemistry. On the formation of stable complexes between He2+ and other simple species: implications for atmospheric and interstellar chemistry”. Journal of Molecular Modeling. 15 (1): 35–40. doi:10.1007/s00894-008-0371-3. PMID 18936986.
  8. ↑ Möller, Thomas; Beland, Michael; Zimmerer, Georg (1985). “Observation of Fluorescence of the HeH Molecule”. Physical Review Letters. 55 (20): 2145–2148. Bibcode:1985PhRvL..55.2145M. doi:10.1103/PhysRevLett.55.2145. PMID 10032060.
  9. ↑ “Wolfgang Ketterle: The Nobel Prize in Physics 2001”.
  10. ↑ Ketterle, W.; Figger, H.; Walther, H. (1985). “Emission spectra of bound helium hydride”. Physical Review Letters. 55 (27): 2941–2944. Bibcode:1985PhRvL..55.2941K. doi:10.1103/PhysRevLett.55.2941. PMID 10032281.
  11. ↑ Lias, S. G.; Liebman, J. F.; Levin, R. D. (1984). “Evaluated Gas Phase Basicities and Proton Affinities of Molecules; Heats of Formation of Protonated Molecules”. Journal of Physical and Chemical Reference Data. 13 (3): 695. Bibcode:1984JPCRD..13..695L. doi:10.1063/1.555719.
  12. 1 2 3 Grandinetti, Felice (tháng 10 năm 2004). “Helium chemistry: a survey of the role of the ionic species”. International Journal of Mass Spectrometry. 237 (2–3): 243–267. Bibcode:2004IJMSp.237..243G. doi:10.1016/j.ijms.2004.07.012.
  13. ↑ Carrington, Alan; Gammie, David I.; Shaw, Andrew M.; Taylor, Susie M.; Hutson, Jeremy M. (1996). “Observation of a microwave spectrum of the long-range He⋯H+
    2 complex”. Chemical Physics Letters. 260 (3–4): 395–405. Bibcode:1996CPL...260..395C. doi:10.1016/0009-2614(96)00860-3.
  14. ↑ Pauzat, F.; Ellinger, Y. (2005). “Where do noble gases hide in space?”. Trong Markwick-Kemper, A. J. (biên tập). Astrochemistry: Recent Successes and Current Challenges (PDF). Poster Book IAU Symposium No. 231. 231. Bibcode:2005IAUS..231.....L. Bản gốc (PDF) lưu trữ ngày 2 tháng 2 năm 2007.
  15. ↑ Fernández, J.; Martín, F. (2007). “Photoionization of the HeH+ molecular ion”. Journal of Physics B. 40 (12): 2471–2480. Bibcode:2007JPhB...40.2471F. doi:10.1088/0953-4075/40/12/020.
  16. ↑ Stutzki, Jürgen; Risacher, Christophe; Ricken, Oliver; Klein, Bernd; Karl Jacobs; Graf, Urs U.; Menten, Karl M.; Neufeld, David; Wiesemeyer, Helmut (tháng 4 năm 2019). “Astrophysical detection of the helium hydride ion HeH+”. Nature. 568 (7752): 357. doi:10.1038/s41586-019-1090-x. PMID 30996316.
  17. ↑ Mannone, F. biên tập (1993). Safety in Tritium Handling Technology. Springer. tr. 92. doi:10.1007/978-94-011-1910-8_4. ISBN 978-94-011-1910-8.
  18. ↑ Harris, G. J.; Lynas-Gray, A. E.; Miller, S.; Tennyson, J. (2004). “The Role of HeH+ in Cool Helium-rich White Dwarfs”. The Astrophysical Journal. 617 (2): L143–L146. arXiv:astro-ph/0411331. Bibcode:2004ApJ...617L.143H. doi:10.1086/427391.
  19. ↑ Liu, X.-W.; Barlow, M. J.; Dalgarno, A.; Tennyson, J.; Lim, T.; Swinyard, B. M.; Cernicharo, J.; Cox, P.; Baluteau, J.-P.; Pequignot, D.; Nguyen, Q. R.; Emery, R. J.; Clegg, P. E. (1997). “An ISO Long Wavelength Spectrometer detection of CH in NGC 7027 and an HeH+ upper limit”. Monthly Notices of the Royal Astronomical Society. 290 (4): L71–L75. Bibcode:1997MNRAS.290L..71L. doi:10.1093/mnras/290.4.l71.
  20. ↑ Neufeld, David A.; Dalgarno, A. (1989). “Fast molecular shocks. I – Reformation of molecules behind a dissociative shock”. Astrophysical Journal. 340: 869–893. Bibcode:1989ApJ...340..869N. doi:10.1086/167441.