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Cited article:
O. Mousis , Y. Alibert , W. Benz
A&A, 449 1 (2006) 411-415
Published online: 2006-03-16
This article has been cited by the following article(s):
21 articles
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Scientific rationale for Uranus and Neptune in situ explorations
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K. E. Mandt, O. Mousis, B. Marty, et al. Comets as Tracers of Solar System Formation and Evolution 297 (2017) https://doi.org/10.1007/978-94-024-1103-4_11
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GAS-PHASE SEQUESTRATION OF NOBLE GASES IN THE PROTOSOLAR NEBULA: POSSIBLE CONSEQUENCES ON THE OUTER SOLAR SYSTEM COMPOSITION
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DETERMINATION OF THE MINIMUM MASSES OF HEAVY ELEMENTS IN THE ENVELOPES OF JUPITER AND SATURN
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Sequestration of Noble Gases by \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 Protoplanetary Disks and Outer Solar System Composition
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