Rossby Wave Instability in Astrophysical Discs
arXiv:1312.4572 · doi:10.1088/0169-5983/46/4/041401
Abstract
A brief review is given of the Rossby wave instability (RWI) in astrophysical discs. In non-self-gravitating discs, around for example a newly forming stars, the instability can be triggered by an axisymmetric bump at some radius in the disc surface mass-density. It gives rise to exponentially growing non-axisymmetric perturbation [, ] in the vicinity of consisting of {\it anticyclonic} vortices. These vortices are regions of high pressure and consequently act to trap dust particles which in turn can facilitate planetesimal growth in proto-planetary discs. The Rossby vortices in the discs around stars and black holes may cause the observed quasi-periodic modulations of the disc's thermal emission.
11 pages, 4 figures
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