State Transitions of Black Hole Accretion Flows
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Abstract
We show that the thermal instability-triggered transition from the state of Shakura-Sunyaev disc to the state of advection-dominated accretion flow is possible for black hole accretion flows composed of two-temperature plasma with bremsstrahlung and synchrotron radiation and Comptonization.
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Cite this article:
LU Ju-Fu, PAN Liu-Bin. State Transitions of Black Hole Accretion Flows[J]. Chin. Phys. Lett., 2001, 18(9): 1294-1296.
LU Ju-Fu, PAN Liu-Bin. State Transitions of Black Hole Accretion Flows[J]. Chin. Phys. Lett., 2001, 18(9): 1294-1296.
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LU Ju-Fu, PAN Liu-Bin. State Transitions of Black Hole Accretion Flows[J]. Chin. Phys. Lett., 2001, 18(9): 1294-1296.
LU Ju-Fu, PAN Liu-Bin. State Transitions of Black Hole Accretion Flows[J]. Chin. Phys. Lett., 2001, 18(9): 1294-1296.
|