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Introduction to Pulsar Wind Nebulae
2016Pulsar Wind Nebulae are nebulae of electrons and positrons powered by a central pulsar. In this chapter I give a detailed description of star evolution, centered on the description of supernova remnants, pulsars and pulsar wind nebulae. The basic properties of pulsars are explained, together with the emission mechanisms responsible for the production ...
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Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit
Nature, 2022Fei Xie +2 more
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Radiative Models of Pulsar Wind Nebulae
2017Since pulsar wind nebulae (PWNe) are the product of the interaction between the magnetized, highly relativistic particle outflow powered by a neutron star’s rotational energy and its surroundings, their emission is sensitive to the properties of the central neutron star, its pulsar wind, and surroundings.
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Modelling the γ-ray pulsar wind nebulae population in our galaxy
Monthly Notices of the Royal Astronomical Society, 2022Michele Fiori, Barbara Olmi, Elena Amato
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Time-dependent modeling of TeV-detected, young pulsar wind nebulae
Journal of High Energy Astrophysics, 2014E De oña wilhelmi
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Pulsar Wind Nebulae with Bow Shocks: Non-thermal Radiation and Cosmic Ray Leptons
Space Science Reviews, 2017Aleksei Petrov +1 more
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Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebulae
Space Science Reviews, 2011Stephen P Reynolds, Fabrizio Bocchino
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