All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{5698f1.ps} \end{figure}$ Figure 1: Number density distribution of stars [**/kpc³] perpendicular to the Galactic plane derived from star counts in CADIS fields. The five fields are coded as: 1 h (squares), 9 h (asterisks), 13 h (circles), 16 h (triangles), 23 h (pentagons). Only data above z = 2 kpc are shown (colour coded in the electronic version). The solid line is the vertical density profile at the position of the Sun of a smooth Galaxy model fitted to the data of the 1 h, 16 h and 23 h fields.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=6.7cm,clip]{5698f2.ps} \end{figure}$ Figure 2: Hess diagram of the 13 h field. The observed distribution of stars in the R - (b-r) plane is colour coded according to the number density of stars per bin of size 0.1 $\times$ 0.1 in magnitude and colour, respectively. The colour table is shown at the top. A smooth model of the Galaxy, which has been fitted to the reference fields, is shown as isodensity contours. The equally spaced contour levels span the same range as the colour table.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=6.7cm,clip]{5698f3.ps} \end{figure}$ Figure 3: The same as Fig. 2 but for the 9 h field.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=6.7cm,clip]{5698f3.ps} \end{figure}$	Figure 3: The same as Fig. 2 but for the 9 h field.
Open with DEXTER