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Magnetic field bending in accretion discs with dynamos

✍ Scribed by C. G. Campbell; J. C. B. Papaloizou; V. Agapitou


Publisher
John Wiley and Sons
Year
1998
Tongue
English
Weight
312 KB
Volume
300
Category
Article
ISSN
0035-8711

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## Abstract The origin of large scale magnetic fields in astrophysical rotators, and the conversion of gravitational energy into radiation near stars and compact objects via accretion have been subjects of active research for a half century. Magnetohydrodynamic turbulence makes both problems highly