$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0542fig1.ps} \end{figure}$ Figure 1: Spacial profile of the H $\beta$ flux (in the units 10^-13 erg cm^-2 s^-1), the [O III]( $\lambda 4659 + \lambda 5007)/\lambda 4363$ ratio (R), and the derived electron temperature along the $\Delta \delta = 30$ $^{\prime \prime }$ N. The position in horizontal axis is relative to the reference star.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.5cm,clip]{0542fig4.ps} \end{figure}$ Figure 4: Apertures of the observations of NGC 346 by: (OCK) this paper, (D75) Dufour (1975), (DH77) Dufour & Harlow (1977), (PTP76) Peimbert & Torres-Peimbert (1976), (P78) Pagel et al. (1978), (P00) Peimbert et al. (2000), and (T03) Tsamis et al. (2003).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.5cm,clip]{0542fig5.ps} \end{figure}$ Figure 5: Linear regression analysis for the data along declination offset $\Delta \delta$ = 0 $^{\prime \prime }$ (squares, solid line) and for the data by Peimbert et al. (2000) (triangles, dashed line). The curved lines define the 95% confidence bands for the regression lines.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0542fig1.ps} \end{figure}$	Figure 1: Spacial profile of the H $\beta$ flux (in the units 10^-13 erg cm^-2 s^-1), the [O III]( $\lambda 4659 + \lambda 5007)/\lambda 4363$ ratio (R), and the derived electron temperature along the $\Delta \delta = 30$ $^{\prime \prime }$ N. The position in horizontal axis is relative to the reference star.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0542fig2.ps} \end{figure}$	Figure 2: Same as Fig. 1, but for $\Delta \delta$ = 0 $^{\prime \prime }$ .
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0542fig3.ps} \end{figure}$	Figure 3: Same as Fig. 1, but for $\Delta \delta$ = 30 $^{\prime \prime }$ S.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=8.5cm,clip]{0542fig4.ps} \end{figure}$	Figure 4: Apertures of the observations of NGC 346 by: (OCK) this paper, (D75) Dufour (1975), (DH77) Dufour & Harlow (1977), (PTP76) Peimbert & Torres-Peimbert (1976), (P78) Pagel et al. (1978), (P00) Peimbert et al. (2000), and (T03) Tsamis et al. (2003).
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=8.5cm,clip]{0542fig5.ps} \end{figure}$	Figure 5: Linear regression analysis for the data along declination offset $\Delta \delta$ = 0 $^{\prime \prime }$ (squares, solid line) and for the data by Peimbert et al. (2000) (triangles, dashed line). The curved lines define the 95% confidence bands for the regression lines.
Open with DEXTER