Communication: Visible line intensities of the triatomic hydrogen ion from experiment and theory-Reference-Cited by-同舟云学术

Communication: Visible line intensities of the triatomic hydrogen ion from experiment and theory

Published:2014-12-28 Issue:24 Volume:141 Page:241104
ISSN:0021-9606
Container-title:The Journal of Chemical Physics
language:en
Short-container-title:The Journal of Chemical Physics

Author:

Petrignani Annemieke¹^ORCID,Berg Max H.¹,Grussie Florian¹,Wolf Andreas¹,Mizus Irina I.²^ORCID,Polyansky Oleg L.²³,Tennyson Jonathan³^ORCID,Zobov Nikolai F.²,Pavanello Michele⁴,Adamowicz Ludwik⁵

Affiliation:

1. Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg, Germany

2. Institute of Applied Physics, Russian Academy of Science, Ulyanov Street 46, Nizhnii Novgorod 603950, Russia

3. Department of Physics and Astronomy, University College London, London WC1E 6BT, United Kingdom

4. Department of Chemistry, Rutgers University, Newark, New Jersey 07102, USA

5. Department of Chemistry and Biochemistry, The University of Arizona, Tucson, Arizona 85721, USA

Funder

European Research Council (ERC)

Russian Foundation for Basic Research (RFBR)

Max-Planck-Gesellschaft (Max Planck Society)

Publisher

AIP Publishing

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy

Link

http://aip.scitation.org/doi/pdf/10.1063/1.4904440

Reference32 articles.

1. Observations of \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\mathrm{H}\,^{+}_{3}$ \end{document} in Dense Molecular Clouds

2. INVESTIGATING THE COSMIC-RAY IONIZATION RATE IN THE GALACTIC DIFFUSE INTERSTELLAR MEDIUM THROUGH OBSERVATIONS OF H+3

3. The role of H3+in planetary atmospheres

4. A stability limit for the atmospheres of giant extrasolar planets

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