Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Keldysh Institute of Applied Mathematics, Moscow
Keldysh Inst. of Applied Mathematics, Moscow, Russia
Keldysh Institute of Applied Mathematics, Moscow;
Keldysh Inst. of Applied Mathematics, Moscow, Russia;
Keldysh Institute of Applied Mathematics, Moscow, Russia
Akademiia Nauk SSSR, Institut Prikladnoi Matematiki, Moscow, USSR
Institut Fiziki Vysokikh Energii, Moscow, USSR
Keldysh Institute of Applied Mathematics, Russian Academy of Sciences
Moscow Physical-Engineering Institute, Moscow, USSRI. V.PanovInstitute of Theoretical and Experimental Physics, Moscow, USSRV. M.ChechetkinInstitute of Applied Mathematics, Moscow, USSR
Institute of Applied Mathematics M.V. Keldysh, Moscow 125047, USSR
M.V. Keldysh Institute of Applied Mathematics, Russian Academy of Sciences
Akademiia Nauk SSSR, Institut Kosmicheskikh Issledovanii, Moscow, USSR
RAN, Inst. Prikladnoj Matematiki
Akademiia Nauk SSSR, Institut Prikladnoi Matematiki, Moscow; Akademiia Nauk SSSR, Institut Fiziki Vysokikh Energii, USSR
Keldysh Institute of Applied Mathematics, Russian Academy of Sciences and ICRAnet Continue Here
AN SSSR, Astronomicheskii Sovet and Institut Prikladnoi Matematiki, Moscow, USSR
Akademiia Nauk SSSR, Institut Kosmicheskikh Issledovanii and Institut Prikladnoi Matematiki, Moscow, USSR
Akademiia Nauk SSSR, Institut Prikladnoi Matematiki and Institut Teoreticheskoi Fiziki, Moscow, USSR
Russian Academy of Sciences, Moscow, Russia
Akademiia Nauk SSSR, Institut Prikladnoi Matematiki; Gosudarstvennyi Komitet po Ispol'zovaniiu Atomnoi Energii, Institut Teoreticheskoi i Eksperimental'noi Fiziki, Moscow, USSR
Institute of Applied Mathematics, U.S.S.R. Academy of Sciences
Institut Fiziki Vysokikh Energii, USSR
3D numerical simulation of gaseous flows structure in semidetached binaries
A possible mechanism for the formation of molecular flows
Astrophysical aspects of antiproton interaction with 4He (antimatter in the universe)
Bipolar flows in the vicinity of a magnetized rotating disk
Boundary Conditions for Simulations of the Thermal Outburst of a Type Ia Supernova
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