activity
19982012
most cited3D numerical simulation of gaseous flows structure in semidetached binaries

136 citations · 356 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2012★ 42 cited

Morphology of the Interaction Between the Stream and Cool Accretion Disk in a Semi-detached Binary Systems

D. V. Bisikalo, A. A. Boyarchuk, P. V. Kaygorodov +1

We analyze heating and cooling processes in accretion disks in binaries. For realistic parameters of the accretion disks in close binaries (with accretion rates from 1e-12 to 1e-7…

astro-ph2006★ 4 cited

Superhumps in Binary Systems and Their Connection to Precessional Spiral Density Waves

P. V. Kaygorodov, D. V. Bisikalo, O. A. Kuznetsov +1

We consider a mechanism for the formation of superhumps in the TV Col system, based on the possible existence of a precessional spiral wave in the accretion disk of the system. Thi…

astro-ph2005★ 16 cited

3D Gasdynamic Modelling of the Changes in the Flow Structure During Transition From Quiescent to Active State in Symbiotic Stars

M. Mitsumoto, B. Jahanara, T. Matsuda +6

The results of 3D modelling of the flow structure in the classical symbiotic system Z~Andromedae are presented. Outbursts in systems of this type occur when the accretion rate exce…

astro-ph2001★ 12 cited

Bending Instability of an Accretion Disc Around a Black Hole

D. Molteni, K. Acharya, Oleg Kuznetsov +2

We demonstrate that generically an accretion disk around a compact object could have a new type of instability in that the accretion flow need not be symmetric with respect to the…

astro-ph2001

TVD Scheme for the Numerical Simulation of the Axisymmetrical Selfgravitating MHD Flows

Alexander E. Dudorov, Oleg A. Kuznetsov, Andrey G. Zhilkin

The explicit quasi-monotonic conservative TVD scheme and numerical method for the solution of the gravitational MHD equations are developed. The 2D numerical code for the simulatio…

astro-ph2000★ 4 cited

Non-conservative Evolution of Cataclysmic Variables

A. V. Fedorova, D. V. Bisikalo, A. A. Boyarchuk +3

We suggest a new mechanism to account for the loss of angular momentum in binaries with non-conservative mass exchange. It is shown that in some cases the loss of matter can result…