アブストラクト |
Accretion discs are behind some of the most fascinating phenomena in
the Universe. Viscous mass transport feed supermassive black holes and
young stars, and accretion discs are sites of both planet formation
and star formation. Keplerian shear flows are linearly unstable in the
presence of a weak magnetic field. The application of this
magnetorotational instability to accretion discs by Balbus |