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• W2897779877 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." @default.
• W2897779877 created "2018-10-26" @default.
• W2897779877 creator A5035516024 @default.
• W2897779877 date "2018-01-01" @default.
• W2897779877 modified "2023-09-27" @default.
• W2897779877 title "Disc Disruption and Accretion Curtains" @default.
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• W2897779877 doi "https://doi.org/10.1007/978-3-319-97646-4_9" @default.
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