All Figures

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig1} \end{figure}$ Figure 1: Density profiles for four of the cases studied. From top to bottom dotted lines correspond to the results of the cases 1, 4, 6 and 7, respectively. Solid lines are fits by the formula of Eq. (1).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig2} \end{figure}$ Figure 2: Triangles show the concentrations predicted by the model studied while the solid line shows the predictions of the toy-model of Bullock et al.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig3} \end{figure}$ Figure 3: Solid lines show the logarithmic slopes of the density profiles given by Eq. (2) for all seven cases studied. From top to bottom, these lines correspond to cases 1, 2, 3, 4, 5, 6 and 7, respectively. Dashed lines show, with the same order, the predictions of the model of Reed et al. (2005), based on the results of their N-body simulations.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.3cm]{5551-fig4} \end{figure}$ Figure 4: Fits of the density profiles of inner regions. From top to bottom dotted lines correspond to the cases 3, 4, 5, 6, 7 of our model while solid lines are the fits by the formula of Eq. (1). The quality of the fit is sufficient for a reasonable estimation of the logarithmic slope.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig5} \end{figure}$ Figure 5: The logarithmic slopes of the density profiles for the cases of Fig. 4. From top to bottom the lines correspond to cases 3, 4, 5, 6, 7. It is clear that larger haloes have at the same radial distance (measured in units of the virial radius) flatter inner density profiles. Additionally, it is clear that $\gamma$ tends asymptotically to values smaller than 0.5.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig6} \end{figure}$ Figure 6: The same as in Fig. 5 but for the outer region. From top to bottom, lines correspond to the cases 1, 2, 3, 4, 5, 6 and 7, respectively. It is clear that the slope $\gamma$ at $R=R_{\rm vir}$ is a decreasing function of the virial mass of the halo.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig7} \end{figure}$ Figure 7: The dependence of the concentration on the mass growth rate of the halo. Triangles represent the concentrations of haloes with large recent mass growth, squares represent the concentrations of all haloes of every case and circles the concentrations of haloes with small recent mass growth.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig8} \end{figure}$ Figure 8: The dependence on the outer slope on the mass growth rate. Solid lines correspond to case 3, dashed lines to case 4 and dotted lines to case 7. Upper lines correspond to haloes with small recent mass growth while lower lines correspond to haloes with large recent mass growth. It is obvious that haloes which recently increased significantly their masses have flatter outer density profiles.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig1} \end{figure}$	Figure 1: Density profiles for four of the cases studied. From top to bottom dotted lines correspond to the results of the cases 1, 4, 6 and 7, respectively. Solid lines are fits by the formula of Eq. (1).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig2} \end{figure}$	Figure 2: Triangles show the concentrations predicted by the model studied while the solid line shows the predictions of the toy-model of Bullock et al.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig3} \end{figure}$	Figure 3: Solid lines show the logarithmic slopes of the density profiles given by Eq. (2) for all seven cases studied. From top to bottom, these lines correspond to cases 1, 2, 3, 4, 5, 6 and 7, respectively. Dashed lines show, with the same order, the predictions of the model of Reed et al. (2005), based on the results of their N-body simulations.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.3cm]{5551-fig4} \end{figure}$	Figure 4: Fits of the density profiles of inner regions. From top to bottom dotted lines correspond to the cases 3, 4, 5, 6, 7 of our model while solid lines are the fits by the formula of Eq. (1). The quality of the fit is sufficient for a reasonable estimation of the logarithmic slope.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig5} \end{figure}$	Figure 5: The logarithmic slopes of the density profiles for the cases of Fig. 4. From top to bottom the lines correspond to cases 3, 4, 5, 6, 7. It is clear that larger haloes have at the same radial distance (measured in units of the virial radius) flatter inner density profiles. Additionally, it is clear that $\gamma$ tends asymptotically to values smaller than 0.5.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig6} \end{figure}$	Figure 6: The same as in Fig. 5 but for the outer region. From top to bottom, lines correspond to the cases 1, 2, 3, 4, 5, 6 and 7, respectively. It is clear that the slope $\gamma$ at $R=R_{\rm vir}$ is a decreasing function of the virial mass of the halo.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{5551-fig7} \end{figure}$	Figure 7: The dependence of the concentration on the mass growth rate of the halo. Triangles represent the concentrations of haloes with large recent mass growth, squares represent the concentrations of all haloes of every case and circles the concentrations of haloes with small recent mass growth.
Open with DEXTER