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An efficient shock-capturing central-type scheme for multidimensional relativistic flows. II. Magnetohydrodynamics
L. Del Zanna, N. Bucciantini, P. Londrillo
A third order shock-capturing numerical scheme for three-dimensional special relativistic magnetohydrodynamics (3-D RMHD) is presented and validated against several numerical tests…
Pulsar bow-shock nebulae. III. Inclusion of a neutral component, and H_{a lpha} luminosity
N. Bucciantini
The interaction of the wind from a pulsar (or more generally from a star) with t he amb ient medium gives rise to the formation of a bow-shock nebula. We present a mode l of adiaba…
An efficient shock-capturing central-type scheme for multidimensional relativistic flows. I. Hydrodynamics
L. Del Zanna, N. Bucciantini
Multidimensional shock-capturing numerical schemes for special relativistic hydrodynamics (RHD) are computationally more expensive than their correspondent Euler versions, due to t…
Pulsar bow-shock nebulae. II. Hydrodynamical simulation
N. Bucciantini
We present hydrodynamical simulations, using a 2-D two component model (ambient medium and pul sar wind have different specific heat ratios), of bow shocks in a representative regi…