An axisymmetric magnetohydrodynamic model for the Crab pulsar wind bubble

• 1 September 1992
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 397, 187-195
• https://doi.org/10.1086/171778

Abstract

Keywords

• CRAB NEBULA
• MAGNETIC FIELD CONFIGURATIONS
• MAGNETOHYDRODYNAMICS
• PULSARS
• SYNCHROTRON RADIATION
• EMISSIVITY
• MAGNETIC FIELD RECONNECTION
• POLARIZED LIGHT
• TORUSES