Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=15.5cm,height=12.5cm]{6934fig1.eps} \end{figure}$ Figure 1: Evolution of chemical abundances in the SBBC model. Vertical axes are the relative abundance and the horizontal axes are relative to the redshift.
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In the text

$\begin{figure} \par\includegraphics[width=15.5cm,height=11.5cm]{6934fig2.eps} \end{figure}$ Figure 2: Evolution of fluorine abundances compared to $\rm {H_2}$ , HD, LiH and $\rm {HeH^+}$ abundances of SBBC model. Vertical axis is the relative abundance when the horizontal axis is relative to the redshift.
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In the text

$\begin{figure} \par\includegraphics[width=15.5cm,height=12.5cm]{6934fig1.eps} \end{figure}$	Figure 1: Evolution of chemical abundances in the SBBC model. Vertical axes are the relative abundance and the horizontal axes are relative to the redshift.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=15.5cm,height=11.5cm]{6934fig2.eps} \end{figure}$	Figure 2: Evolution of fluorine abundances compared to $\rm {H_2}$ , HD, LiH and $\rm {HeH^+}$ abundances of SBBC model. Vertical axis is the relative abundance when the horizontal axis is relative to the redshift.
Open with DEXTER