Accretion disks in the cataclysmic variables
The general equations describing the time-independent structure of gaseous circumstellar disks in vertical hydrostatic equilibrium are derived. The possibility of turbulent instablilty and the resulting viscosity laws are discussed.
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Format: | Dissertation |
Language: | English |
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University of Cape Town
2016
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Online Access: | http://hdl.handle.net/11427/18880 |