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- W2618930892 abstract "Context. Mass transfer due to Roche lobe overflow leads to the formation of an accretion disk around a weakly magnetized white dwarf (WD) in cataclysmic variables. At the inner edge of the disk, the gas comes upon the surface of the WD and has to get rid of its excess kinetic energy in order to settle down on the more slowly rotating outer stellar layers. This region is known as the boundary layer (BL)." @default.
- W2618930892 created "2017-06-05" @default.
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- W2618930892 date "2017-09-01" @default.
- W2618930892 modified "2023-10-16" @default.
- W2618930892 title "The vertical structure of the boundary layer around compact objects" @default.
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- W2618930892 doi "https://doi.org/10.1051/0004-6361/201730847" @default.
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