States and State Transitions in Low Mass X-Ray Binaries
We investigate the model of a disk/coronal accretion flow into a black hole. We build a numerical code to ascertain whether the inner regions of an accretion disk in X-ray binaries can transform from a cool standard disk to an advection-dominated flow through the known properties of Coulomb interact...
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| Format: | Others |
| Language: | en |
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LSU
2009
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| Online Access: | http://etd.lsu.edu/docs/available/etd-07072009-123333/ |