Titlebook: High Energy Density Laboratory Astrophysics; G.A. Kyrala Book 2005 Springer Science+Business Media B.V. 2005 Accretion.MHD.Plasma.astrophy

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https://doi.org/10.1007/1-4020-4162-4Accretion; MHD; Plasma; astrophysics; relativistic jet

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Asymmetric Supernovae: Yes, Rotation and Magnetic Fields are Important,henomena are at work involving rotation and magnetic fields. We summarize the importance of the magnetorotational instability for the core collapse problem and sketch some of the effects that large magnetic fields, ∼10. G, may have on the physics of the supernova explosion.

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Radiative Shock Experiments at LULI,designed targets filled with xenon gaz at low pressure, the propagation of a strong shock with a radiative precursor is evidenced. The main measured quantities related to the shock (electronic density, propagation velocities, temperature, radial dimension) are presented and compared with various numerical simulations.

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Analytical Study of Supernova Remnant Non-Stationary Expansions, by blowing pulsar wind. The most dangerous perturbations correspond to wavelengths comparable to the shell thickness. We analyze the fragility of the supernova remnant shell in function of the initial perturbation amplitude and the shell thickness.

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Laboratory Simulations of Supernova Shockwave Propagation,to the heated gas. The second shock remains visible and continues to expand. A minimum condition for the formation of the second shock is that the original shock is super-critical, i.e., the temperature distribution ahead of the original shock has an inflexion point. In a non-radiative control exper