Modeling the Dynamical and Radiative Evolution of a Pulsar Wind Nebula inside a Supernova Remnant

Details Modeling the Dynamical and Radiative Evolution of a Pulsar Wind Nebula inside a Supernova Remnant Modeling the Dynamical and Radiative Evolution of a Pulsar Wind Nebula inside a Supernova Remnant

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe..38g&link_type=abstract

Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo

Computer Science

Compact Objects

Scientific paper

A pulsar wind nebula inside a supernova remnant offers a unique insight into the properties of neutron stars, pulsar winds, and the progenitor supernova. However, this is complicated by the rapid and complicated evolution such a pulsar wind nebulae undergoes. In this talk, I will present a model for the dynamical and radiative evolution of a pulsar wind nebulae inside a remnant which can extract the desired information from observations, and demonstrate its success in reproducing the total radio to X-ray spectrum of the Crab Nebula.

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