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Multi-wavelength study of High Mass X-ray Binaries

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Figure

FIGURE 1. Optical to MIR SEDs of IGR J16318-4848 (left) and IGR J17544-2619 (right), including data from ESO/NTT, VISIR on VLT/UT3 and Spitzer [11]
FIGURE 2. Corbet diagram, adapted and taken from Liu et al. [24], showing the relation between orbital and spin periods
FIGURE 3. Scenarios illustrating two possible configurations of INTEGRAL sources: a NS orbiting a supergiant star on a circular orbit (left image); and on an eccentric orbit (right image), accreting from the clumpy stellar wind of the supergiant

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