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Accretion in supergiant High Mass X-ray Binaries

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Figure

Figure 1. Density distribution (in gr cm−3; color bar) on the orbital plane after ∼ 3 orbits
Figure 2. Left: Time-averaged simulated absorbing column density (NH) for various neutron star masses
Figure 4. Left: Simulated light-curve of Vela X-1 together with a sine wave of 6820 sec period (red dashed line).This quasi-periodic modulations was observed in Vela X-1 by [17]

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