2-D MHD Configurations for Accretion Disks Around Magnetized Stars

Details 2-D MHD Configurations for Accretion Disks Around Magnetized Stars 2-D MHD Configurations for Accretion Disks Around Magnetized Stars

2009-12-09

arxiv.org/abs/0912.1721v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

3 pages, 1 figure, presentation given at the Marcel Grossman Meeting XII, July 12 - 18 2009 (Paris)

Scientific paper

We discuss basic features of steady accretion disk morphology around
magnetized compact astrophysical objects. A comparison between the standard
model of accretion based on visco-resistive MHD and the plasma instabilities,
like ballooning modes, triggered by very low value of resistivity, is proposed.

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