Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae

Details Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae

2007-10-03

arxiv.org/abs/0710.0844v1

AIPConf.Proc.983:216-218,2008

Astronomy and Astrophysics

Astrophysics

3 pages, 7 figures, proceeding of the conference "40 Years of Pulsars ", 12-17 August 2007, Montreal, Canada, submitted to AIP

Scientific paper

10.1063/1.2900146

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 and spectral index simulated maps in comparison to observations. The time dependent relativistic magnetohydrodynamic (RMHD) equations are solved with a shock capturing code together with the evolution of the maximum particles energy. Applications to Pulsar Wind Nebulae (PWNe) are shown.

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