We show a complete set of diagnostic tools aimed at reproducing synthetic synchrotron emissivity, polarization and spectral index simulated maps in comparison to observations. A numerical shock capturing code is used to evolve relativistic MHD and emitting particle maximum energy equations in time and space. We apply the method to Pulsar Wind Nebulae.
Synchrotron emission simulated maps: Pulsar Wind Nebulae / D. Volpi; L. Del Zanna; E. Amato; N. Bucciantini. - In: MEMORIE DELLA SOCIETÀ ASTRONOMICA ITALIANA. - ISSN 1824-016X. - STAMPA. - 78:(2007), pp. 662-664.
Synchrotron emission simulated maps: Pulsar Wind Nebulae
DEL ZANNA, LUCA;E. Amato;
2007
Abstract
We show a complete set of diagnostic tools aimed at reproducing synthetic synchrotron emissivity, polarization and spectral index simulated maps in comparison to observations. A numerical shock capturing code is used to evolve relativistic MHD and emitting particle maximum energy equations in time and space. We apply the method to Pulsar Wind Nebulae.
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