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- W2106996985 abstract "This article discusses close binary systems with orbital periods of a few hours, in which a compact primary star accretes mass from a low-mass companion. If the primary is a white dwarf these are called cataclysmic variables (CVs); if it is a neutron star or black hole the systems are known as low mass X-ray binaries (LMXBs). The evolution of these systems has been reviewed by many authors, and the interested reader is referred to these papers (e.g. King, 1988) for further details." @default.
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- W2106996985 date "1990-01-01" @default.
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- W2106996985 title "Mass Transfer and Evolution in Close Binaries" @default.
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- W2106996985 doi "https://doi.org/10.1007/978-3-642-76238-3_2" @default.
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