21 citations · 48 across the 5 of their papers we have counts for
5 papers
Simulated non-thermal emission from SNR G1.9+0.3
Marco A. Villagran, D. O. Gómez, P. F. Velázquez +7
Supernova remnants are the nebular leftover of defunct stellar environments, resulting from the interaction between a supernova blastwave and the circumstellar medium shaped by the…
A 3D MHD simulation of SN 1006: a polarized emission study for the turbulent case
P. F. Velázquez, E. M. Schneiter, E. M. Reynoso +6
Three dimensional magnetohydrodynamical simulations were carried out in order to perform a new polarization study of the radio emission of the supernova remnant SN 1006. These simu…
Two-fluid turbulence including electron inertia
Nahuel Andrés, Carlos Gonzalez, Luis Martin +2
We present a full two-fluid magnetohydrodynamic (MHD) description for a completely ionized hydrogen plasma, retaining the effects of the Hall current, electron pressure and electro…
Kelvin-Helmholtz versus Hall Magneto-shear instability in astrophysical flows
Daniel O. Gomez, Cecilia Bejarano, Pablo D. Mininni
We study the stability of shear flows in a fully ionized plasma. Kelvin-Helmholtz is a well known, macroscopic and ideal shear-driven instability. In sufficiently low density plasm…
Energy spectrum, dissipation and spatial structures in reduced Hall magnetohydrodynamic
L. N. Martin, P. Dmitruk, D. O. Gomez
We analyze the effect of the Hall term in the magnetohydrodynamic turbulence under a strong externally supported magnetic field, seeing how this changes the energy cascade, the cha…