The cooling of astrophysical media by H2
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/305/4/802/18632079/305-4-802.pdf
Reference17 articles.
1. Quantum‐mechanical Study of Ro‐vibrational Transitions in H \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 $_{2}$ \end{document} Induced by He Atoms
2. Temporal evolution of MHD shocks in the interstellar medium
3. Rotational excitation of hydrogen molecules by hydrogen atoms
4. A quantal study of the rovibrational excitation of by H
5. Rovibrational relaxation in collisions between molecules: I. Transitions induced by ground state para-
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