All Figures

$\begin{figure} \includegraphics[width=8.4cm,clip]{1455fig1.eps} \end{figure}$ Figure 1: The colour- $\sigma _0$ relations for Nop galaxies (circles and fitted lines), and Pec objects (stars). The calculated regressions for the Nop subsample are shown. In V-J and V-K, part of the "peculiar'' objects tend to be bluer than "normal''. This effect is lessened in the high mass range, and much reduced in J-H and J-K.
Open with DEXTER

In the text

$\begin{figure} \includegraphics[width=8.4cm,clip]{1455fig1.eps} \end{figure}$	Figure 1: The colour- $\sigma _0$ relations for Nop galaxies (circles and fitted lines), and Pec objects (stars). The calculated regressions for the Nop subsample are shown. In V-J and V-K, part of the "peculiar'' objects tend to be bluer than "normal''. This effect is lessened in the high mass range, and much reduced in J-H and J-K.
Open with DEXTER