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X-Ray Emission from the Guitar Nebula

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©1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Roger W. Romani et al 1997 ApJ 484 L137 DOI 10.1086/310796

1538-4357/484/2/L137

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 ~ 107 eV particles in the pulsar wind and constrains the properties of the postshock 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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10.1086/310796