All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3550.f1.ps} \end{figure}$ Figure 1: Convergence of constrained $\Lambda$ -iterations. Results of 20 temperature iterations starting from an isothermal stratification with T = 5000 K are plotted for a simulation with ${\cal N} = 4 \times 10^{5}$ packets. The solution for the conical radiation field is plotted as open circles.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3550.f2.ps} \end{figure}$ Figure 2: Convergence of constrained $\Lambda$ -iterations. Results of 20 level population iterations starting from Saha-Boltzmann populations at T = 5000 K are plotted for the mass shell m = 10 in a simulation with ${\cal N} = 4 \times 10^{5}$ packets. The solution for the conical radiation field is plotted as open circles.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3550.f3.ps} \end{figure}$ Figure 3: Test of departure coefficients b_i. Results obtained at iteration 20 in Monte Carlo calculation with ${\cal N} = 4 \times 10^{5}$ packets are plotted as solid lines for the indicated levels. The solutions for the conical radiation field are plotted as filled circles (i=2), open circles (i=3) and asterisks (i=10).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3550.f4.ps} \end{figure}$ Figure 4: Monte Carlo spectrum obtained at iteration 20 in Monte Carlo calculation with ${\cal N} = 4 \times 10^{5}$ packets. The unit of luminosity density is 10⁴⁵ erg s^-1 cm^-1. The rest wavelengths of H $\alpha$ , H $\beta$ and H $\gamma$ are indicated.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3550.f1.ps} \end{figure}$	Figure 1: Convergence of constrained $\Lambda$ -iterations. Results of 20 temperature iterations starting from an isothermal stratification with T = 5000 K are plotted for a simulation with ${\cal N} = 4 \times 10^{5}$ packets. The solution for the conical radiation field is plotted as open circles.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3550.f2.ps} \end{figure}$	Figure 2: Convergence of constrained $\Lambda$ -iterations. Results of 20 level population iterations starting from Saha-Boltzmann populations at T = 5000 K are plotted for the mass shell m = 10 in a simulation with ${\cal N} = 4 \times 10^{5}$ packets. The solution for the conical radiation field is plotted as open circles.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3550.f3.ps} \end{figure}$	Figure 3: Test of departure coefficients b_i. Results obtained at iteration 20 in Monte Carlo calculation with ${\cal N} = 4 \times 10^{5}$ packets are plotted as solid lines for the indicated levels. The solutions for the conical radiation field are plotted as filled circles (i=2), open circles (i=3) and asterisks (i=10).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3550.f4.ps} \end{figure}$	Figure 4: Monte Carlo spectrum obtained at iteration 20 in Monte Carlo calculation with ${\cal N} = 4 \times 10^{5}$ packets. The unit of luminosity density is 10⁴⁵ erg s^-1 cm^-1. The rest wavelengths of H $\alpha$ , H $\beta$ and H $\gamma$ are indicated.
Open with DEXTER