Radial Shocks in Advection-Dominated Accretion FlowsAround Black Holes
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Abstract
We have solved the set of equations for advection-dominated accretion flows (ADAFs) around black holes, and found a new class of global solutions with standing radial shocks.Such α-X-type shocks may exist in flows when 0 ≤ α < 0.05. An example solution is given explicitly, for which α=0.01 and γ=1.5. The shock position is Rsh=8.68Rg, which is between the inner sonic point Rs1=3.88Rg and the outer sonic point Rs2=85.92Rg.
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Cite this article:
GU Wei-Min, LU Ju-Fu. Radial Shocks in Advection-Dominated Accretion FlowsAround Black Holes[J]. Chin. Phys. Lett., 2001, 18(1): 148-150.
GU Wei-Min, LU Ju-Fu. Radial Shocks in Advection-Dominated Accretion FlowsAround Black Holes[J]. Chin. Phys. Lett., 2001, 18(1): 148-150.
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GU Wei-Min, LU Ju-Fu. Radial Shocks in Advection-Dominated Accretion FlowsAround Black Holes[J]. Chin. Phys. Lett., 2001, 18(1): 148-150.
GU Wei-Min, LU Ju-Fu. Radial Shocks in Advection-Dominated Accretion FlowsAround Black Holes[J]. Chin. Phys. Lett., 2001, 18(1): 148-150.
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