Instability in the Magnetized Accretion Disks with Outflows in the Presence of Self-Gravity

We study the stability of a model of magnetized accretion disk, in whichoutflows play a significant role in driving the inflow, and magnetic field is generated bya dynamo operating in the disk. We present a local and linear analysis of the stabilityin the presence of self-gravity and winds. The numerical results show the model withself-gravity is unstable in all parts, while in a model without self-gravity, instabilitycan be observed only in regions near the central body. Eventually, the effect of windcooling on the model stability was discussed. According to the results, in systemswithout self-gravity, wind cooling can help the system towards stability, but in thepresence of self-gravity, it is shown that our model will remain unstable in all regions.Comparison of these result with observational evidence shows that this model can besuitable for the explaining the behavior of the disks surrounding young stellar objects.