The emerging population of pulsar wind nebulae in hard X-rays

Fabio Mattana; Diego Götz; Régis Terrier; Matthieu Renaud; Maurizio Falanga

doi:10.1063/1.3149427

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arXiv · 0903.1192

The emerging population of pulsar wind nebulae in hard X-rays

Fabio Mattana·Diego Götz·Régis Terrier·Matthieu Renaud·Maurizio Falanga

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Abstract

The hard X-ray synchrotron emission from pulsar wind nebulae (PWNe) probes energetic particles, closely related to the pulsar injection power at the present time. INTEGRAL has disclosed the yet poorly known population of hard X-ray pulsar/PWN systems. We summarize the properties of the class, with emphasys on the first hard X-ray bow-shock (CTB 80 powered by PSR B1951+32), and highlight some prospects for the study of Pulsar Wind Nebulae with the Simbol-X mission.

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Fabio Mattana, Diego Götz, Régis Terrier, Matthieu Renaud, Maurizio Falanga. 2009-03-06. The emerging population of pulsar wind nebulae in hard X-rays. https://doi.org/10.1063/1.3149427

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