Astronomy & Astrophysics

$\begin{figure} \par\resizebox{7.5cm}{!}{\includegraphics[clip=true,angle=0]{7234fig1.eps}}\end{figure}$ Figure 1: The observed intensity spectra (solid line) are plotted over on the fit (crosses) obtained using a grid of synthetic spectra based on the Holweger-Müller model computed with SYNTHE. Delbouille refers to the Delbouille intensity spectrum, Neckel to the Neckel intensity spectrum (see text for details).
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In the text

$\begin{figure} \par\resizebox{7.5cm}{!}{\includegraphics[clip=true,angle=0]{7234fig2.eps}}\end{figure}$ Figure 2: 3D abundance corrections: each correction is located according the parameters ( $T_{\rm eff}$ and [Fe/H]) of the related model; the models have very similar gravity ( $\ensuremath{\log\ensuremath{g}}$ in between 4.44 and 4.50). Black numbers depict the 3D-1D LHD differences, grey (green in colour) ones the 3D-1D internal model differences.
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In the text

$\begin{figure} \par\resizebox{7.5cm}{!}{\includegraphics[clip=true,angle=0]{7234fig3.ps}}\end{figure}$ Figure 3: Average temperature structures of 3D $\ensuremath {{\rm CO}^5{\rm BOLD}}$ (solid lines) in comparison to 1D LHD (dotted lines) models. The lower pair of curves is for 5770 K/4.44/0.0 (solar) models, the upper pair for 5900 K/4.50/-3.0 models. For clarity, the later models were shifted by +2000 K.
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In the text

$\begin{figure} \par\resizebox{7.5cm}{!}{\includegraphics[clip=true,angle=0]{7234fig1.eps}}\end{figure}$	Figure 1: The observed intensity spectra (solid line) are plotted over on the fit (crosses) obtained using a grid of synthetic spectra based on the Holweger-Müller model computed with SYNTHE. Delbouille refers to the Delbouille intensity spectrum, Neckel to the Neckel intensity spectrum (see text for details).
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$\begin{figure} \par\resizebox{7.5cm}{!}{\includegraphics[clip=true,angle=0]{7234fig2.eps}}\end{figure}$	Figure 2: 3D abundance corrections: each correction is located according the parameters ( $T_{\rm eff}$ and [Fe/H]) of the related model; the models have very similar gravity ( $\ensuremath{\log\ensuremath{g}}$ in between 4.44 and 4.50). Black numbers depict the 3D-1D LHD differences, grey (green in colour) ones the 3D-1D internal model differences.
Open with DEXTER

$\begin{figure} \par\resizebox{7.5cm}{!}{\includegraphics[clip=true,angle=0]{7234fig3.ps}}\end{figure}$	Figure 3: Average temperature structures of 3D $\ensuremath {{\rm CO}^5{\rm BOLD}}$ (solid lines) in comparison to 1D LHD (dotted lines) models. The lower pair of curves is for 5770 K/4.44/0.0 (solar) models, the upper pair for 5900 K/4.50/-3.0 models. For clarity, the later models were shifted by +2000 K.
Open with DEXTER