In two temperature plasmas, one regime seen in the formation of these is derived by ignoring some of the electron-ion relaxation processes. Another model of their formation is based on magnetic fields creating turbulence meaning that viscosity will scale with the alpha factor. These objects that are subject to the Balbus-Hawley instability are described by advection dominated regimes and the (*) Shakura-Sunyaev model. These power X-ray pulsars. The upper bound of their formation rate is given by the Eddington limit. Angular momentum is transferred outwards in these. These objects are usually accompanied by relativistic jets and all quasars and black holes are surrounded by these objects. For 10 points, name this fla
In two temperature plasmas, one regime seen in the formation of these is derived by ignoring some of the electron-ion relaxation processes. Another model of their formation is based on magnetic fields creating turbulence meaning that viscosity will scale with the alpha factor. These objects that are subject to the Balbus-Hawley instability are described by advection dominated regimes and the (*) Shakura-Sunyaev model. These power X-ray pulsars. The upper bound of their formation rate is given by the Eddington limit. Angular momentum is transferred outwards in these. These objects are usually accompanied by relativistic jets and all quasars and black holes are surrounded by these objects. For 10 points, name this flat grouping of matter that surrounds a gravitational source.
In two temperature plasmas, one regime seen in the formation of these is derived by ignoring some of the electron-ion relaxation processes.