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27 April 2024

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Results 1 to 19 of 19 for query "V. M. Chechetkin". (0.00 sec.)

Spherical Bondi accretion onto a magnetic dipole
Yu. M. Toropin; O. D. Toropina; M. M. Romanova; V. V. Savelyev; V. M. Chechetkin; R. V. E. Lovelace;
17 Nov 1998

Structure of gaseous flows in semidetached binaries after mass transfer termination
D.V.Bisikalo; A.A.Boyarchuk; A.A.Kilpio; O.A.Kuznetsov; V.M.Chechetkin;
14 Feb 2001 / Astron. Zh. 2001, v.78, pp.707-716 (Astron. Reports, v.45, pp.611-619)

Driven-disk model for binaries with precessing donor star. Three-dimensional simulations
D.V.Bisikalo; A.A.Boyarchuk; O.A.Kuznetsov; V.M.Chechetkin;
24 Mar 2000 / Astron. Zh. 1999, v.76, p.672 (Astron. Reports v.43, p.587)

Three-dimensional modeling of mass transfer in close binary systems with non-synchronous rotation
D.V. Bisikalo; A.A. Boyarchuk; O.A. Kuznetsov; V.M. Chechetkin;
31 Dec 1998 / Astron. Zh. 1999, v.76, p.270 (Astron. Reports v.43, p.229)

The Influence of Parameters on the Flow Structure in Semidetached Binary Systems: 3D Numerical Simulation
D.V.Bisikalo; A.A.Boyarchuk; O.A.Kuznetsov; V.M.Chechetkin;
1 Jun 1998 / Astron. Zh. 1998, v.75, p.706 (Astron. Reports v.42, p.621)

3D numerical simulation of gaseous flows structure in semidetached binaries
D. V. Bisikalo; A. A. Boyarchuk; V. M. Chechetkin; O. A. Kuznetsov; D. Molteni;
20 May 1998 / MNRAS, 1998, v.300, No.1, p.39

Hydrodynamic Simulations of Counterrotating Accretion Disks
O.A.Kuznetsov; R.V.E.Lovelace; M.M.Romanova; V.M.Chechetkin;
27 Oct 1998 / ApJ, v.514, p.691

Magneto-centrifugally driven winds: comparison of MHD simulations with theory
G.V. Ustyugova; A.V. Koldoba; M.M. Romanova; V.M. Chechetkin; R.V.E. Lovelace;
15 Dec 1998

Synthetic Doppler maps of gaseous flows in semidetached binaries based on the results of 3D gas dynamical simulations
D.V.Bisikalo; A.A.Boyarchuk; O.A.Kuznetsov; V.M.Chechetkin;
22 Nov 2000

10.

The impact of viscosity on the morphology of gaseous flows in semidetached binary systems
D.V.Bisikalo; A.A.Boyarchuk; O.A.Kuznetsov; V.M.Chechetkin;
7 Jul 1999 / Astron.Rep. 44 (2000) 26; Astron.Zh.Akad.Nauk SSSR 77 (2000) 31

11.

Comparison of 2D and 3D models of flow structure in semidetached binaries
D.V.Bisikalo; A.A.Boyarchuk; V.M.Chechetkin; O.A.Kuznetsov; D.Molteni;
7 Jul 1999 / Astron.Rep. 43 (1999) 797; Astron.Zh.Akad.Nauk SSSR 76 (1999) 905

12.

Evidence for the Absence of a Stream-Disk Shock Interaction (Hot Spot) in Semi-Detached Binary Systems. Comparison of Numerical Simulation Results and Observations
D.V.Bisikalo; A.A.Boyarchuk; O.A.Kuznetsov; T.S.Khruzina; A.M.Cherepashchuk; V.M.Chechetkin;
11 Feb 1998 / Astron. Reports, 1998, 42, 33

13.

Impact of a Binary System Common Envelope on Mass Transfer through the Inner Lagrange Point
D.V.Bisikalo; A.A.Boyarchuk; O.A.Kuznetsov; V.M.Chechetkin;
3 Feb 1998 / Astron. Reports, 1997, 41, 794

14.

Three-dimensional Modeling of the Matter Flow Structure in Semidetached Binary Systems
D.V.Bisikalo; A.A.Boyarchuk; O.A.Kuznetsov; V.M.Chechetkin;
1 Feb 1998 / Astron. Reports, 1997, 41, 786

15.

Cosmic voids and the kinetic analysis
V.G.Gurzadyan; N.N.Fimin; V.M.Chechetkin;
1 Sep 2022

16.

On the origin of cosmic web
V.G.Gurzadyan; N.N.Fimin; V.M.Chechetkin;
18 Jan 2022

17.

Orbital evolution of a binary neutron star and gravitational radiation
Kuznetsov O.A.; Prokhorov M.E.; Sazhin M.V.; Chechetkin V.M.;
22 Dec 1998 / Astron.Rep. 42 (1998) 638-648

18.

Influence of dark matter on gravitational stability of isothermal gas clouds
I.Yu. Kalashnikov; V.M. Chechetkin;
24 Feb 2022

19.

The modified Newton attraction law and its connection with cosmological $Λ$--term
N.N. Fimin; V.M. Chechetkin;
9 Dec 2020

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