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X-ray Emission from the Guitar Nebula

Roger W. Romani·James M. Cordes·I. -A. Yadigaroglu
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Abstract

We have detected weak soft X-ray emission from the Pulsar Wind Nebula trailing the high velocity star PSR 2224+65 (the `Guitar Nebula'). This X-ray flux gives evidence of γ~10^7 eV particles in the pulsar wind and constrains the properties of the post-shock flow. The X-ray emission is most easily understood if the shocked pulsar wind is partly confined in the nebula and if magnetic fields in this zone can grow to near equipartition values.

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Roger W. Romani, James M. Cordes, I. -A. Yadigaroglu. 1997-06-20. X-ray Emission from the Guitar Nebula. https://doi.org/10.1086/310796

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