374 research outputs found
The structure of cool accretion disc in semidetached binaries
We present the results of qualitative consideration of possible changes
occurring during the transition from the hot accretion disc to the cool one. We
argue the possible existence of one more type of spiral density waves in the
inner part of the disc where gasdynamical perturbations are negligible. The
mechanism of formation of such a wave as well as its parameters are considered.
We also present the results of 3D gasdynamical simulation of cool accretion
discs. These results confirm the hypothesis of possible formation of the spiral
wave of a new, "precessional" type in the inner regions of the disc. Possible
observational manifestations of this wave are discussed.Comment: LaTeX, 16 pages, 8 figures, to be published in Astron. Z
The impact of viscosity on the morphology of gaseous flows in semidetached binary systems
Results of 3D gas dynamical simulation of mass transfer in binaries are
presented for systems with various values of viscosity. Analysis of obtained
solutions shows that in the systems with low value of viscosity the flow
structure is qualitatively similar to one for systems with high viscosity.
Presented calculations confirm that there is no shock interaction between the
stream from L1 and the forming accretion disk (`hot spot') at any value of
viscosity.Comment: LaTeX, 18 pages, 15 eps-figures, Astron. Reports, in pres
Features of the mass transfer in magnetic cataclysmic variables with fast-rotating white dwarfs
The flow structure in magnetic cataclysmic variables was investigated taking
into account the effects of strong magnetic field and fast rotation of the
white dwarf. We modeled the AE Aqr system as a unique object that has the
rotation period of the white dwarf is about 1000 times shorter than the orbital
period of the binary system. Observations show that in spite of fast rotation
of the white dwarf some part of the stream from the inner Lagrange point comes
into the Roche lobe region. We analyzed possible mechanisms preventing material
to outflow from the system.Comment: 5 pages, 6 figures. Proceedings of the Conference "Physics at the
Magnetospheric Boundary" (Geneva, Switzerland, 25 - 26 June, 2013), to be
published in "EPJ Web of Conferences
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