Astronomy & Astrophysics

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$\begin{figure}\par\includegraphics[width=8.8cm,clip]{0377fig1.eps} \end{figure}$ Figure 1: Energy loss rate of electrons with kinetic energy E due to bremsstrahlung according to Eq. (9) (H) and according to the approximation of Blumenthal and Gould (BG), compared with the energy loss rate by e-e collisions (coll. loss) in a completely ionized plasma with hydrogen number density $N_{\rm H}=1$ cm^-3 and ratio $N_{\rm He}/N_{\rm H}=0.1$ .
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In the text

$\begin{figure}\par\includegraphics[width=8.8cm,clip]{0377fig1.eps} \end{figure}$	Figure 1: Energy loss rate of electrons with kinetic energy E due to bremsstrahlung according to Eq. (9) (H) and according to the approximation of Blumenthal and Gould (BG), compared with the energy loss rate by e-e collisions (coll. loss) in a completely ionized plasma with hydrogen number density $N_{\rm H}=1$ cm^-3 and ratio $N_{\rm He}/N_{\rm H}=0.1$ .
Open with DEXTER