All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0308fig1.eps} \end{figure}$ Figure 1: Polarization of the stars within $20\hbox {$^\circ $ }$ area of the South Galactic Pole. The length of the bar gives the amount of polarization, its direction gives the direction of the polarization plane. The dots are the stars with P₀ = 0.0.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0308fig2.eps} \end{figure}$ Figure 2: The same as Fig. 1, but for the North Galactic Pole. Markkanen's cloud is also shown.
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In the text

$\begin{figure} \par\includegraphics[width=7.4cm,clip]{0308fig3.eps} \end{figure}$ Figure 3: Distribution of the polarization directions in the equatorial coordinate system for the NGP ( upper plot) and SGP ( lower plot). The maxima at $70\hbox {$^\circ $ }$ in the north direction and $130\hbox {$^\circ $ }$ in the south direction correspond to $53\hbox {$^\circ $ }$ and $83\hbox {$^\circ $ }$ in the Galactic coordinate frame.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0308fig4.eps} \end{figure}$ Figure 4: Dependence of the polarization on distance for the NGP and SGP areas.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0308fig5.eps} \end{figure}$ Figure 5: Median line of the polarization - distance dependence calculated by binning the distances for the NGP (dashed line) and SGP (solid line). Vertical bars are $2\sigma$ errors computed from the dispersion.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0308fig1.eps} \end{figure}$	Figure 1: Polarization of the stars within $20\hbox {$^\circ $ }$ area of the South Galactic Pole. The length of the bar gives the amount of polarization, its direction gives the direction of the polarization plane. The dots are the stars with P₀ = 0.0.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0308fig2.eps} \end{figure}$	Figure 2: The same as Fig. 1, but for the North Galactic Pole. Markkanen's cloud is also shown.
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$\begin{figure} \par\includegraphics[width=7.4cm,clip]{0308fig3.eps} \end{figure}$	Figure 3: Distribution of the polarization directions in the equatorial coordinate system for the NGP ( upper plot) and SGP ( lower plot). The maxima at $70\hbox {$^\circ $ }$ in the north direction and $130\hbox {$^\circ $ }$ in the south direction correspond to $53\hbox {$^\circ $ }$ and $83\hbox {$^\circ $ }$ in the Galactic coordinate frame.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{0308fig4.eps} \end{figure}$	Figure 4: Dependence of the polarization on distance for the NGP and SGP areas.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{0308fig5.eps} \end{figure}$	Figure 5: Median line of the polarization - distance dependence calculated by binning the distances for the NGP (dashed line) and SGP (solid line). Vertical bars are $2\sigma$ errors computed from the dispersion.
Open with DEXTER