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Breathing Life Into Dead-Zones
2013
EPJ Web of Conferences
The terrestrial planet formation regions of protoplanetary disks are generally sufficiently cold to be con-sidered non-magnetized and, consequently, dynamically inactive. However, recent investigations of these so-called "Dead-Zones" indicate the possibility that disks with strong mean radial temperature gradients can support instabilities associated with disk-normal gradients of the basic Keplerian shear profile. This process, known as the Goldreich-Schubert-Fricke (GSF) instability, is the
doi:10.1051/epjconf/20134603003
fatcat:moa5j546rbg4rdqhivn2uyo3nu