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- W1979349721 abstract "The boundary layer between the accretion disc and white dwarf in non-magnetic cataclysmic variables is the major source of X-rays from these systems. Two modes of X-ray emission exist; at low accretion rates a thermal instability develops in the accreting matter and a hard X-ray emitting corona is formed around the white dwarf; at high accretion rates a cool, very soft X-ray emitting boundary layer is formed. Hard and soft X-ray observations of cataclysmic variables with a boundary layer are described and compared with theory. Emphasis is put on the new insight we have gained from the observations with the EXOSAT observatory." @default.
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- W1979349721 date "1988-01-01" @default.
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- W1979349721 title "Accretion disc boundary layers with white dwarfs" @default.
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- W1979349721 doi "https://doi.org/10.1016/0273-1177(88)90416-4" @default.
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