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Sulphur abundances from the S i near-infrared triplet at 1045 nm

E. Caffau, R. Faraggiana, P. Bonifacio, H.-G. Ludwig and M. Steffen
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Astronomy & Astrophysics 456 (2) 697 (2006)
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Energy transport, overshoot, and mixing in the atmospheres of M-type main- and pre-main-sequence objects

H.-G. Ludwig, F. Allard and P. H. Hauschildt
Astronomy & Astrophysics 459 (2) 599 (2006)
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The Inverse‐ \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 $\textsf{C}$\end{document} Shape of Solar Chromospheric Line Bisectors

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The Astrophysical Journal 639 (1) 516 (2006)
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The dynamics of the solar chromosphere: comparison of model predictions with millimeter-interferometer observations

M. Loukitcheva, S. K. Solanki and S. White
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