Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae

Simple item page
dc.creatorVolpi, Delia
dc.creatorDel Zanna, Luca
dc.creatorAmato, Elena
dc.creatorBucciantini, Niccolo
dc.date2007-10-03
dc.date.accessioned2026-07-07T11:19:45Z
dc.date.available2026-07-07T11:19:45Z
dc.descriptionWe 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.
dc.description3 pages, 7 figures, proceeding of the conference "40 Years of Pulsars ", 12-17 August 2007, Montreal, Canada, submitted to AIP
dc.identifierhttps://arxiv.org/abs/0710.0844
dc.identifierhttp://arxiv.org/abs/0710.0844
dc.identifierAIPConf.Proc.983:216-218,2008
dc.identifierdoi:10.1063/1.2900146
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193795
dc.subjectAstrophysics
dc.titleSimulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae
dc.typetext

Files

Collections

arXiv