Pradhan HMXB Illustration (IMAGE)

Penn State

Pradhan HMXB Illustration

Caption

Illustration of a high-mass X-ray binary system made up of a compact, incredibly dense neutron star paired with a massive 'normal' supergiant star. New data from NASA's Chandra X-ray Observatory shows that the neutron star in the high-mass X-ray binary, OAO 1657-415, passed through a dense patch of stellar wind from its companion star, demonstrating the clumpy nature of stellar winds.

Credit

NASA/CXC/M.Weiss

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