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The Astrophysical Journal 799 (1) 66 (2015)
DOI: 10.1088/0004-637X/799/1/66
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\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 Diffuse Interstellar Clouds: A Tracer for the Cosmic‐Ray Ionization Rate

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The Astrophysical Journal 671 (2) 1736 (2007)
DOI: 10.1086/523036
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HD molecules at high redshift

P. Noterdaeme, P. Petitjean, C. Ledoux, R. Srianand and A. Ivanchik
Astronomy & Astrophysics 491 (2) 397 (2008)
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Connecting the primordial and Galactic deuterium abundances

G. Steigman, D. Romano and M. Tosi
Monthly Notices of the Royal Astronomical Society 378 (2) 576 (2007)
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The Galactic deuterium abundance and dust depletion: insights from an expanded Ti/H sample★

Sara L. Ellison, Jason X. Prochaska and Sebastian Lopez
Monthly Notices of the Royal Astronomical Society 380 (3) 1245 (2007)
DOI: 10.1111/j.1365-2966.2007.12192.x
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