Up: Stellar disks and embedded

Appendix A: Appendix A

The results of the photometric decomposition of the 28 galaxies are shown in this appendix. The figures follow the same order of the list of objects in Table 1. The upper left panel shows the surface brightness profiles of each galaxy along the major and minor axes (filled squares), the same profiles of the bulge (crosses) and the disk profile along the major axis (full line), all plotted vs. a^1/4. The same profiles plotted vs. the semi-major axis $\it a$ are shown in the upper right panel. In the left lower panels are shown: the ellipticity 1-b/a, $a_3/a\, \cdot$ 100, $a_4/a\, \cdot$ 100, and $a_6/a\, \cdot$ 100 profiles before (filled squares) and after (crosses) disk subtraction. At the right lower panels: the position angle PA, $b_3/a\, \cdot$ 100 $b_4/a\, \cdot$ 100 and $b_6/a\, \cdot$ 100 before (filled squares) and after (crosses) disk subtraction.

Acknowledgements

We wish to honour the memory of our dear friend and coinvestigator in this project Dr. Jean-Luc Nieto whose enthusiasm and scientific curiosity we still miss. CS thanks R. Michard for his unpublished data on NGC 3585. This work was supported by the DFG (Sonderforschungsbereich SFB 328 and SFB 375).

$\begin{figure} \includegraphics[width=11.6cm,clip]{a1.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a2.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a3.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a4.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a5.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a6.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a7.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a8.ps}\end{figure}$

$\begin{figure} \includegraphics[width=11.6cm,clip]{a9.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a10.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a11.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a12.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a13.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a14.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a15.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a16.ps}\end{figure}$

$\begin{figure} \includegraphics[width=11.6cm,clip]{a17.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a18.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a19.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a20.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a21.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a22.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a23.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a24.ps}\end{figure}$

$\begin{figure} \includegraphics[width=11.6cm,clip]{a25.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a26.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a27.ps}\end{figure}$ $\begin{figure} \includegraphics[width=11.6cm,clip]{a28.ps}\end{figure}$

Up: Stellar disks and embedded

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