Instability of anomalous viscosity disks around young stellar objects

Details Instability of anomalous viscosity disks around young stellar objects Instability of anomalous viscosity disks around young stellar objects

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jplph..73..367y&link_type=abstract

Journal of Plasma Physics, vol. 73, Issue 03, p.367-375

Physics

Plasma Physics

Scientific paper

An accretion disk with vertical structure around a young stellar object is investigated, considering anomalous magnetic viscosity. It was found that the I-mode was unstable in the outer disk, and sometimes turned stable in the inner disk, for the standard α model. However, we find that the I-mode is always unstable in the inner disk, owing to the anomalous magnetic viscosity.

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