$\begin{figure} \par\includegraphics[angle=270,width=16.4cm,clip]{4720fig1.ps} \end{figure}$ Figure 1: The absolutely fluxed 3500-7800 Å low resolution spectrum of Nova Scuti 2005 N.2 observed on 2005 Oct. 27.76 UT. Most probable identification for the emission lines is given. The ordinate scale is logarithmic to emphasize the visibility of weaker features.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4720fig2.ps} \end{figure}$ Figure 2: Resolved H $\alpha$ and OI 8446 Å emission profiles of Nova Scuti 2005 N.2 observed on 2005 Oct. 27.74 UT. The continuum is normalized to 1.0. The numbers identify the ripples in the profiles whose radial velocity is given in Table 2.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4720fig3.ps} \end{figure}$ Figure 3: The photometric evolution of Nova Scuti 2005 N.2. The dots mark our CCD observations in Table 1, the crosses correspond to B, V band integration over the absolutely fluxed spectrum of Fig. 1, and the open circles are values published in IAUC 8617. The dashed line is hand drawn.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=16.4cm,clip]{4720fig1.ps} \end{figure}$	Figure 1: The absolutely fluxed 3500-7800 Å low resolution spectrum of Nova Scuti 2005 N.2 observed on 2005 Oct. 27.76 UT. Most probable identification for the emission lines is given. The ordinate scale is logarithmic to emphasize the visibility of weaker features.
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$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4720fig2.ps} \end{figure}$	Figure 2: Resolved H $\alpha$ and OI 8446 Å emission profiles of Nova Scuti 2005 N.2 observed on 2005 Oct. 27.74 UT. The continuum is normalized to 1.0. The numbers identify the ripples in the profiles whose radial velocity is given in Table 2.
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$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4720fig3.ps} \end{figure}$	Figure 3: The photometric evolution of Nova Scuti 2005 N.2. The dots mark our CCD observations in Table 1, the crosses correspond to B, V band integration over the absolutely fluxed spectrum of Fig. 1, and the open circles are values published in IAUC 8617. The dashed line is hand drawn.
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