Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=15.8cm,clip]{MS2939f1.ps}\end{figure}$ Figure 1: Distribution of the IPS and 7C radio sources. The IPS radio sources are shown by hexagons of 30' diameter, the 7C radio sources - by filled squares of increasing size for intervals of flux density: <0.5, 0.5-1, 1-2, >2 Jy.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{MS2939f2.ps}\end{figure}$ Figure 2: Distribution of the deconvolved major axis size for single FIRST counterparts (solid line) and most compact component for double FIRST counterparts (dashed line).
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In the text

$\begin{figure} \par\includegraphics[width=15.8cm,clip]{MS2939f1.ps}\end{figure}$	Figure 1: Distribution of the IPS and 7C radio sources. The IPS radio sources are shown by hexagons of 30' diameter, the 7C radio sources - by filled squares of increasing size for intervals of flux density: <0.5, 0.5-1, 1-2, >2 Jy.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{MS2939f2.ps}\end{figure}$	Figure 2: Distribution of the deconvolved major axis size for single FIRST counterparts (solid line) and most compact component for double FIRST counterparts (dashed line).
Open with DEXTER