F.Pauzat and Y. Ellinger Where do noble gases hide in space?Archiválva2007. február 2-i dátummal a Wayback Machine-ben, Astrochemistry: Recent Successes and Current Challenges, Poster Book IAU Symposium No. 231, 2005 A. J. Markwick-Kemper (ed.)
doi.org
dx.doi.org
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 Data13 (3), 695. o. DOI:10.1063/1.555719.
J. Fernandez; F. Martin (2007). „Photoionization of the HeH+ molecular ion”. Journal of Physics B: At. Mol. Opt. Phys40 (12), 2471–2480. o. DOI:10.1088/0953-4075/40/12/020.
Coxon, J (1999). „Experimental Born–Oppenheimer Potential for theX1Σ+Ground State of HeH+: Comparison with theAb InitioPotential”. Journal of Molecular Spectroscopy193 (2), 306–318. o. DOI:10.1006/jmsp.1998.7740. PMID9920707.
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 Modeling15 (1), 35–40. o. DOI:10.1007/s00894-008-0371-3. PMID18936986.
Alan Carrington, David I. Gammie, Andrew M. Shaw, Susie M. Taylor and Jeremy M. Hutson (1996). „Observation of a microwave spectrum of the long-range He···H2+ complex”. Chemical Physics Letters260 (3–4), 395–405. o. DOI:10.1016/0009-2614(96)00860-3.
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 Society357 (2), 471–477. o. DOI:10.1111/j.1365-2966.2005.08611.x.
Harris, G.J., Lynas-Gray, A.E.; Miller, S.; Tennyson, J. (2004). „The Role of HeH+ in Cool Helium-rich White Dwarfs”. The Astrophysical Journal617 (2), L143–L146. o. DOI:10.1086/427391.
Neufeld, David A., Dalgarno, A. (1989). „Fast molecular shocks. I – Reformation of molecules behind a dissociative shock”. Astrophysical Journal340, 869–893. o. DOI:10.1086/167441.
Coxon, J (1999). „Experimental Born–Oppenheimer Potential for theX1Σ+Ground State of HeH+: Comparison with theAb InitioPotential”. Journal of Molecular Spectroscopy193 (2), 306–318. o. DOI:10.1006/jmsp.1998.7740. PMID9920707.
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 Modeling15 (1), 35–40. o. DOI:10.1007/s00894-008-0371-3. PMID18936986.
F.Pauzat and Y. Ellinger Where do noble gases hide in space?Archiválva2007. február 2-i dátummal a Wayback Machine-ben, Astrochemistry: Recent Successes and Current Challenges, Poster Book IAU Symposium No. 231, 2005 A. J. Markwick-Kemper (ed.)