All Figures

$\begin{figure} {\psfig{figure=0170f1.ps,width=8.5cm,clip=} }\end{figure}$ Figure 1: Zero-gravity surface around the Local Group now (solid line) and 12.5 Gyr ago (dashed line).
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In the text

$\begin{figure} {\psfig{figure=0170f2.ps,width=18cm,clip=} }\end{figure}$ Figure 2: The phase portrait of the the very local Hubble flow: radial velocity vs. radial distance plots for 22 galaxies of the flow - solid lines. For comparison: same for trajectories calculated with the same initial conditions 12.5 Gyr ago, but without cosmic vacuum - dashed lines. Circles indicate the present state.
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In the text

$\begin{figure} {\psfig{figure=0170f3.ps,width=18cm,angle=-90,clip=} }\end{figure}$ Figure 3: Velocity-distance ratio for the galaxies of the very local Hubble flow as a function of time.
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In the text

$\begin{figure} {\psfig{figure=0170f4.ps,width=18cm,angle=-90,clip=} }\end{figure}$ Figure 4: For comparison: same for trajectories calculated with the same initial conditions 12.5 Gyr ago, but without cosmic vacuum.
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In the text

$\begin{figure} {\psfig{figure=0170f1.ps,width=8.5cm,clip=} }\end{figure}$	Figure 1: Zero-gravity surface around the Local Group now (solid line) and 12.5 Gyr ago (dashed line).
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$\begin{figure} {\psfig{figure=0170f2.ps,width=18cm,clip=} }\end{figure}$	Figure 2: The phase portrait of the the very local Hubble flow: radial velocity vs. radial distance plots for 22 galaxies of the flow - solid lines. For comparison: same for trajectories calculated with the same initial conditions 12.5 Gyr ago, but without cosmic vacuum - dashed lines. Circles indicate the present state.
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$\begin{figure} {\psfig{figure=0170f3.ps,width=18cm,angle=-90,clip=} }\end{figure}$	Figure 3: Velocity-distance ratio for the galaxies of the very local Hubble flow as a function of time.
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$\begin{figure} {\psfig{figure=0170f4.ps,width=18cm,angle=-90,clip=} }\end{figure}$	Figure 4: For comparison: same for trajectories calculated with the same initial conditions 12.5 Gyr ago, but without cosmic vacuum.
Open with DEXTER