Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae
Journal Article
·
· AIP Conference Proceedings
- Dipartimento di Astronomia e Scienza dello Spazio-Largo Fermi 2-50125 Firenze (Italy)
- INAF-Osservatorio Astrofisico di Arcetri-Largo Fermi 5-50125 Firenze (Italy)
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.
- OSTI ID:
- 21136717
- Journal Information:
- AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 983; ISSN 0094-243X; ISSN APCPCS
- Country of Publication:
- United States
- Language:
- English
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