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Paper: Distribution of Patterns and Flow Dynamics in Accreting White Dwarfs
Volume: 469, 18th European White Dwarf Workshop (EUROWD12)
Page: 359
Authors: Boneva, D.; Filipov, L.
Abstract: In the diversity of white dwarf stars population it is clear that the behavior of the disc flow is not common and uniform for all the close binary stars. It is quite affected both by the influences of mass transfer parameters: velocity and density, and by gravitational tidal effects. We aim to examine and compare the morphology of whole disc's flows, implying the data of DN and DA types of white dwarfs in the calculations. It is employed with two different numerical codes and box-framed schemes in the models are proposed. The results demonstrate of how the dense patterns and waves evolve in the studying types of white dwarfs. An effect of their development to the whole disc's shape and inner structure configuration is shown. We find a close relation between cooling–heating processes in the binary system and the patterns distribution there.
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