Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{2625fig1.eps} \end{figure}$ Figure 1: Scattering density distribution of ISM (m-extended medium, s-thin screen medium).
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In the text

$\begin{figure} \par\includegraphics[width=7.1cm,clip]{2625fig2.eps} \end{figure}$ Figure 2: Theoretical structure functions and observations of PSR B0833-45. a) $C_{-4,{\rm s}}$ is treated as a free parameter: the dashed, solid, and dotted lines represent $C_{-4,{\rm s}}=10^{3.8}$ , 10^4.2, and 10^4.6 ${\rm m}^{-20/3}$ , respectively. b) $L_{\rm s}$ is treated as a free parameter: the dashed, solid, and dotted lines represent $L_{\rm s}=0.2$ , 0.4, and 0.48 kpc, respectively. Note: Solid dots are observational data from S2000. Solid lines represent theoretical results by the adoption of the best parameters listed in line 1 of Table 1. Dashed and dotted lines show the influence of variation in one parameter on the structure function, while all the other parameters were kept constant in accordance with Table 1.
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In the text

$\begin{figure} \par\includegraphics[width=6.9cm,clip]{2625fig3.eps} \end{figure}$ Figure 3: Theoretical structure functions and observations of PSR B0833-45. The solid line represents the two-component model of the ISM, and the dashed and dotted lines the single extended medium model with $\beta =11/3$ and $\beta =4$ , respectively.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{2625fig1.eps} \end{figure}$	Figure 1: Scattering density distribution of ISM (m-extended medium, s-thin screen medium).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=6.9cm,clip]{2625fig3.eps} \end{figure}$	Figure 3: Theoretical structure functions and observations of PSR B0833-45. The solid line represents the two-component model of the ISM, and the dashed and dotted lines the single extended medium model with $\beta =11/3$ and $\beta =4$ , respectively.
Open with DEXTER