Magnetohydrodynamic winds and jets from accretion disks

dc.creatorSpruit, H. C.
dc.date1996-02-05
dc.date.accessioned2026-07-07T02:20:52Z
dc.date.available2026-07-07T02:20:52Z
dc.descriptionThe theory of magnetically accelerated outflows and jets from accretion disks is reviewed at an introductory level, with special attention to problem areas like the launching conditions of the flow at the disk surface, stability of the magnetic field, and collimation mechanisms. This text will appear in R.A.M.J. Wijers, M.B. Davies and C.A. Tout, eds., Physical processes in Binary Stars, Kluwer Dordrecht, 1996 (NATO ASI series).
dc.description40 pages, 14 ps figures. Also available at ftp://ibm-3.mpa-garching.mpg.de/pub/suh/henk2.ps.gz or at ftp://ibm-3.mpa-garching.mpg.de/pub/suh/henk1.ps.gz (higher quality figures, bigger file)
dc.identifierhttps://arxiv.org/abs/astro-ph/9602022
dc.identifierhttp://arxiv.org/abs/astro-ph/9602022
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10357
dc.subjectAstrophysics
dc.titleMagnetohydrodynamic winds and jets from accretion disks
dc.typetext

Files

Collections