318 citations · 575 across the 5 of their papers we have counts for
13 papers
Non-thermal emission from relativistic MHD simulations of PWNe: from synchrotron to inverse Compton
D. Volpi, L. Del Zanna, E. Amato +1
In this paper we complete the set of diagnostic tools for synchrotron emitting sources presented by Del Zanna et al. (Astron. Astrophys. 453, 621, 2006) with the computation of inv…
Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae
Delia Volpi, Luca Del Zanna, Elena Amato +1
We present a complete set of diagnostic tools aimed at reproducing synthetic non-thermal (synchrotron and/or Inverse Compton, IC) emissivity, integrated flux energy, polarization a…
Proper motions of radiative knots in simulations of stellar jets - An alternative to pulsating inflow conditions
F. Rubini, S. Lorusso, L. Del Zanna +1
Elongated jets from young stellar objects typically present a nodular structure, formed by a chain of bright knots of enhanced emission with individual proper motions. Though it is…
ECHO: an Eulerian Conservative High Order scheme for general relativistic magnetohydrodynamics and magnetodynamics
L. Del Zanna, O. Zanotti, N. Bucciantini +1
We present a new numerical code, ECHO, based on an Eulerian Conservative High Order scheme for time dependent three-dimensional general relativistic magnetohydrodynamics (GRMHD) an…
Simulated synchrotron emission from Pulsar Wind Nebulae
Luca Del Zanna, Delia Volpi, Elena Amato +1
A complete set of diagnostic tools aimed at producing synthetic synchrotron emissivity, polarization, and spectral index maps from relativistic MHD simulations is presented. As a f…
Relativistic MHD simulations of pulsar bow-shock nebulae
N. Bucciantini, E. Amato, L. Del Zanna
Pulsar bow-shock nebulae are a class of pulsar wind nebulae (PWNe) that form when the pulsar wind is confined by the ram pressure of the ambient medium, and are usually associated…