All Figures

$\begin{figure} \par\psfig{file=3661fg01.eps,width=8.8cm}\end{figure}$ Figure 1: The morphology-radius relation. We show the cumulative radial distribution for the 5 galaxy types: Eb (ellipticals with M_R < -22), E (other ellipticals), S0 galaxies and early and late spirals (Se and Sl). The radial distributions of Eb and Sl galaxies are significantly different from the three other distributions.
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In the text

$\begin{figure} \par\psfig{file=3661fg02.eps,width=8.8cm}\end{figure}$ Figure 2: The morphology-radius relation, expressed as the fraction of galaxies of different types for various projected distances (with H₀ = 100 km s^-1 Mpc^-1) . The dashed lines were taken from Fig. 4 in WGJ, and the symbols represent our results.
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In the text

$\begin{figure} \par\psfig{file=3661fg03.eps,width=8.8cm}\end{figure}$ Figure 3: The morphology-density relation using $\Sigma _{10}$ , the projected density derived from the 10-th nearest neighbour. We show the cumulative distribution of $\Sigma _{10}$ for the various galaxy classes. Note that the brightest ellipticals are not included in the elliptical class.
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In the text

$\begin{figure} \par\psfig{file=3661fg04.eps,width=8.8cm}\end{figure}$ Figure 4: The morphology-density relation in the traditional representation, i.e. as the variation of the fraction of galaxies of different morphological types with projected density $\Sigma _{10}$ .
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In the text

$\begin{figure} \par\psfig{file=3661fg05.eps,width=8.5cm}\end{figure}$ Figure 5: The distribution of the galaxies w.r.t $\Sigma _{10}$ and R/r₂₀₀ ( top) and $\Sigma _{1}$ and R/r₂₀₀ ( bottom). $\Sigma _{10}$ is the projected density derived from the 10-th nearest neighbour while $\Sigma _{1}$ is derived from the projected distance to the nearest neighbour.
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In the text

$\begin{figure} \par\psfig{file=3661fg06.eps,width=8.8cm}\end{figure}$ Figure 6: The morphology-density relation using $\Sigma _{1}$ , the projected density derived from the nearest neighbour. We show the cumulative distribution of $\Sigma _{1}$ for the various galaxy classes.
Open with DEXTER

In the text

$\begin{figure} \par\psfig{file=3661fg01.eps,width=8.8cm}\end{figure}$	Figure 1: The morphology-radius relation. We show the cumulative radial distribution for the 5 galaxy types: Eb (ellipticals with M_R < -22), E (other ellipticals), S0 galaxies and early and late spirals (Se and Sl). The radial distributions of Eb and Sl galaxies are significantly different from the three other distributions.
Open with DEXTER

$\begin{figure} \par\psfig{file=3661fg02.eps,width=8.8cm}\end{figure}$	Figure 2: The morphology-radius relation, expressed as the fraction of galaxies of different types for various projected distances (with H₀ = 100 km s^-1 Mpc^-1) . The dashed lines were taken from Fig. 4 in WGJ, and the symbols represent our results.
Open with DEXTER

$\begin{figure} \par\psfig{file=3661fg03.eps,width=8.8cm}\end{figure}$	Figure 3: The morphology-density relation using $\Sigma _{10}$ , the projected density derived from the 10-th nearest neighbour. We show the cumulative distribution of $\Sigma _{10}$ for the various galaxy classes. Note that the brightest ellipticals are not included in the elliptical class.
Open with DEXTER

$\begin{figure} \par\psfig{file=3661fg04.eps,width=8.8cm}\end{figure}$	Figure 4: The morphology-density relation in the traditional representation, i.e. as the variation of the fraction of galaxies of different morphological types with projected density $\Sigma _{10}$ .
Open with DEXTER

$\begin{figure} \par\psfig{file=3661fg05.eps,width=8.5cm}\end{figure}$	Figure 5: The distribution of the galaxies w.r.t $\Sigma _{10}$ and R/r₂₀₀ ( top) and $\Sigma _{1}$ and R/r₂₀₀ ( bottom). $\Sigma _{10}$ is the projected density derived from the 10-th nearest neighbour while $\Sigma _{1}$ is derived from the projected distance to the nearest neighbour.
Open with DEXTER

$\begin{figure} \par\psfig{file=3661fg06.eps,width=8.8cm}\end{figure}$	Figure 6: The morphology-density relation using $\Sigma _{1}$ , the projected density derived from the nearest neighbour. We show the cumulative distribution of $\Sigma _{1}$ for the various galaxy classes.
Open with DEXTER