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Theory of Pulsar Winds

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arxiv astro-ph/0201439 v1 pith:ILHHWTRG submitted 2002-01-27 astro-ph

Jonathan Arons This is my paper · ORCID
classification astro-ph
keywords energywindscentralcompactconverteddiscussemissiongets
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I discuss recent work on the nature of relativistic winds from Rotation Powered Pulsars, on the physics of how they transport energy from the central compact object to the surrrounding world, and how that energy gets converted into observable synchrotron emission.

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Cited by 1 Pith paper

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  1. Combined VERITAS and NuSTAR observations of the gamma-ray binary HESS J0632+057

    astro-ph.HE 2019-08 conditional novelty 5.0 of 10

    New NuSTAR and VERITAS spectra of HESS J0632+057 are well fitted by a pulsar-wind shock model, yielding a degenerate constraint with wind magnetization around 0.003 to 0.03 at the shock.

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