Radial equation for an accretion flow driven by Poynting flux

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dc.creatorLee, Hyun Kyu
dc.date2002-02-06
dc.date2002-02-07
dc.date.accessioned2026-07-07T11:28:52Z
dc.date.available2026-07-07T11:28:52Z
dc.descriptionUsing a toy model of a two dimensional accretion disk, we discuss further the radial equation of the accretion flow dominated by the Poynting flux. Assuming the force-free condition is valid around the accretion disk, the relation between the fluid angular velocity of the disk, $Ω_D$, and the angular velocity of the magnetic field lines, $Ω_F$, is also discussed.
dc.description11 pages, typos corrected
dc.identifierhttps://arxiv.org/abs/astro-ph/0202113
dc.identifierhttp://arxiv.org/abs/astro-ph/0202113
dc.identifierJ.KoreanPhys.Soc.40:934-937,2002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196534
dc.subjectAstrophysics
dc.titleRadial equation for an accretion flow driven by Poynting flux
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