Jets and Disk-Winds from Pulsar Magnetospheres

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dc.creatorLovelace, Richard V. E.
dc.creatorTurner, Leaf
dc.creatorRomanova, Marina M.
dc.date2006-10-03
dc.date.accessioned2026-07-07T10:40:20Z
dc.date.available2026-07-07T10:40:20Z
dc.descriptionWe discuss axisymmetric force-free pulsar magnetospheres with magnetically collimated jets and a disk-wind obtained by numerical solution of the pulsar equation. This solution represents an alternative to the quasi-spherical wind solutions where a major part of the current flow is in a current sheet which is unstable to magnetic field annihilation.
dc.description6 figures, accepted for publication in the ApJ
dc.identifierhttps://arxiv.org/abs/astro-ph/0610087
dc.identifierhttp://arxiv.org/abs/astro-ph/0610087
dc.identifierAstrophys.J.652:1494-1498,2006
dc.identifierdoi:10.1086/508413
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181310
dc.subjectAstrophysics
dc.titleJets and Disk-Winds from Pulsar Magnetospheres
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