Skip to main content

and
  1. No Access

    Chapter and Conference Paper

    3D Accretion Discs Dynamics: Numerical simulations

    D. V. Bisikalo in Chaos in Astronomy (2009)

  2. No Access

    Chapter and Conference Paper

    Fully developed turbulence in accretion discs of binary stars: turbulent viscosity coefficient and power spectrum.

    A. M. Fridman, D. V. Bisikalo, A. A. Boyarchuk, L. Pustil’nik in Chaos in Astronomy (2009)

  3. No Access

    Chapter

    On Possible Nature of Pre-eclipse Dips in Light Curves of Semi-detached Systems with Steady-state Disks

    In order to explain pre-eclipse dips at phases ∼0.7 in light curves of cataclysmic variables, the hypothesis of the thickening at the outer edge of the accretion disk is usually used. Shock-free nature of the ...

    D. V. Bisikalo, P. V. Kaygorodov in Close Binaries in the 21st Century: New Op… (2006)

  4. No Access

    Chapter and Conference Paper

    The Morphology of Gaseous Flows in Z and in the Active State

    E. Yu. Kilpio, D. V. Bisikalo, A. A. Boyarchuk, O. A. Kuznetsov in Astrophysical disks (2006)

  5. No Access

    Chapter and Conference Paper

    Morphology of the Interaction between the Stream and Cool Accretion Disc in Semidetached Binaries

    P. V. Kaigorodov, D. V. Bisikalo, A. A. Boyarchuk, O. A. Kuznetsov in Astrophysical disks (2006)

  6. No Access

    Chapter and Conference Paper

    Disc Formation in Binary be Stars

    D. V. Bisikalo, A. A. Boyarchuk, P. Harmanec, P. V. Kaigorodov in Astrophysical disks (2006)

  7. No Access

    Chapter

    Numerical Modeling of Mass Transfer in Close Binaries

    The review of gasdynamic models used for the description of the mass exchange in close binaries is presented. Main features of the flow structure are summarized. Special attention is paid to physics of accreti...

    D.V. Bisikalo in Zdeněk Kopal’s Binary Star Legacy (2005)

  8. No Access

    Chapter

    Summary of Quantitative Interpretation of IMAGE Far Ultraviolet Auroral Data

    Direct imaging of the magnetosphere by instruments on the IMAGE spacecraft is supplemented by simultaneous observations of the global aurora in three far ultraviolet (FUV) wavelength bands. The purpose of the ...

    H. U. Frey, S. B. Mende, T. J. Immel in Magnetospheric Imaging — The Image Prime M… (2003)