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Figure 1:
The bulk Lorentz factor of the flow as a function of radius for different
values of ![]() ![]() |
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Figure 2:
The bulk Lorentz factor dependence on the cooling efficiency of the flow and jet opening angles.
The solid curves correspond to the fast kink case while the dashed to the slow kink one.
The black, red and green curves correspond to fast cooling, slow cooling and jet opening angle
of ![]() |
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Figure 3:
The dependence of the magnetization parameter on the radius
for the different prescriptions of radiative cooling and the instability
timescale. Notice that the flow becomes matter-dominated at distances greater than ![]() |
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Figure 4:
The bulk Lorentz factor of the flow for different ![]() ![]() |
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![]() |
Figure 5:
The bulk Lorentz factor of the flow for different jet opening angles ![]() |
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![]() |
Figure 6:
The magnetization ![]() ![]() ![]() ![]() ![]() |
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![]() |
Figure 7:
The radiative efficiency of the flow, defined as the ratio of the radiated luminosity
over the luminosity of the flow for different ![]() ![]() ![]() ![]() ![]() |
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