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Broad-band aperiodic variability in X-ray pulsars: accretion rate fluctuations propagating under the influence of viscous diffusion

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Figure

Figure 1. The broadband aperiodic variability of the accretion luminosity in XRPs is originated from the variability of the mass accretion rate, which is initially produced in the disc
Figure 2. Zones in an accretion disc for different mass accretion rates ˙ M . Inner disc radii for surface magnetic field strengths of 10 11 and 10 12 G are represented by black dashed lines (the magnetic field is assumed to be dipole and the coefficient Λ
Figure 4. The absolute value of the transfer functions |G M ˙ (f, R, R ′ )|
Figure 7. The absolute value of the transfer function |G M ˙ (f, R = 1, R ′ )|
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