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Disc Disruption and Accretion Curtains

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Book cover Magnetohydrodynamics in Binary Stars

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 456))

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Abstract

The intermediate polars, some X-ray binary pulsars and the accreting millisecond pulsars have magnetic primary stars accreting from a partially disrupted disc via an inner magnetically channelled curtain flow. The stellar magnetic field and the associated magnetosphere interact with the disc in a way which is affected by the strength of its magnetic diffusivity. For sufficiently large η values, the stellar poloidal field lines remain closed and linked to the disc. For smaller values of η field line opening can occur and wind flows can result from the disc and the primary star. Angular momentum can be transported in a variety of ways.

Field lines inside the corotation radius tend to remain closed and the disc becomes disrupted as a result of vertical expansion due to magnetic heating. Expanding material can be accelerated through a sonic point and then flow through a magnetically channelled curtain region to accrete on to the star through a narrow shock region. A detailed study of disc disruption and the curtain flow is presented here.

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Campbell, C.G. (2018). Disc Disruption and Accretion Curtains. In: Magnetohydrodynamics in Binary Stars. Astrophysics and Space Science Library, vol 456. Springer, Cham. https://doi.org/10.1007/978-3-319-97646-4_9

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