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Time-dependent modelling of pulsar wind nebulae

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arxiv 1308.1626 v1 pith:DSST35HD submitted 2013-08-07 astro-ph.HE

M.J. Vorster , O. Tibolla , S.E.S. Ferreira , S. Kaufmann This is my paper · ORCID
classification astro-ph.HE
keywords modelpulsarwindhessnebulanebulaesourcesunidentified
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A spatially-independent model that can be used to calculate the temporal evolution of the electron/ positron spectrum in a spherically expanding pulsar wind nebula is presented. The model is applied to the young nebula G21.5-0.9, as well as to the unidentified TeV sources HESS J1427-608 and HESS J1507-622. The parameters derived from the model strengthens the idea that the unidentified sources can be identified as evolved pulsar wind nebulae.

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