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A Magnetic Model for Low/Hard States Associated with Jets in Black Hole X Ray Binaries

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Figure

Figure 1. A schematic drawing of disc-corona model with magnetic patches.
Table 2. Fitting results of X-ray luminosity and jet power for five BHXBs.
Figure 2. The spectral profiles of the LH state of five BHXBs are plotted in zigzag lines, which are superposition of thermal and power law components in solid and dashed lines, respectively
Figure 3. The relation between LX and LJ in the rising phase of the LH state of five BHXBs
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