Low star formation efficiency due to turbulent adiabatic compression in the Taffy bridge

The mean-square separation be- tween particle pairs is plotted against time for fifty different initial separations at a turbulence level of R λ = 815, with the

In doing so, we will highlight the fact that the velocity field u plays a special role in (1), in that we will require different levels of regularity on u and b to prove a

We prove that if the initial magnetic field decays sufficiently fast, then the plasma flow behaves as a solution of the free nonstationnary Navier–Stokes equations when |x| → +∞,

l’utilisation d’un remède autre que le médicament, le mélange de miel et citron était le remède le plus utilisé, ce remède était efficace dans 75% des cas, le

Selecting the 120 kHz frequency bandwidth of the filter it is ¾ spectrum magnitude of the analysis signals and central frequencies of the filter are left the same: 150 kHz,

Integrating the power spectral densities of the magnetic and electric fields in the 10 to 500 Hz frequency range shows that the energy density of waves is higher inside the

We present measurements of sound velocity and absorption obtained by Brillouin light scattering which show that the effect of structural relaxation is not observed at

* The speed upper limit for real particles in the imaginary spacetime is , because the relativistic expression of the mass shows that the velocity of real particles cannot be