Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
ITEP Moscow
ITEP, Moscow
Akademiia Nauk SSSR, Institut Prikladnoi Matematiki, Moscow, USSR
Akademiia Nauk SSSR, Institut Teoreticheskoi i Eksperimental'noi Fiziki, Moscow, USSR
Radioastrofizicheskaia Observatoriia, Riga, Latvian SSR; Institut Teoreticheskoi i Eksperimental'noi Fiziki, Moscow, USSR
Institut Fiziki Vysokikh Energii, Moscow, USSR
Gosudarstvennyi Komitet po Ispol'zovanniu Atomnoi Energii, Institut Teoreticheskoi i Eksperimental'noi Fiziki, Moscow, USSR
Institute of Applied Mathematics U.S.S.R. Academy of Sciences
Institut Teoreticheskoi Fiziki, Moscow, USSR
Institute for Theoretical and Experimental Physics
Institute of Theoretical and Experimental Physics
Institut Teoreticheskoi i Eksperimental'noi Fiziki, Moscow, Russia
Alikhanov Institute for Theoretical and Experimental Physics
Akademiia Nauk SSSR, Institut Eksperimental'noi i Teoreticheskoi Fiziki, Moscow, USSR
Inst. Teoreticheskoj i Ehksperimental'noj Fiziki
Akademiia Nauk SSSR, Institut Prikladnoi Matematiki, Moscow; Akademiia Nauk SSSR, Institut Fiziki Vysokikh Energii, USSR
Institute of Applied Mathematics, AS USSR
AN SSSR, Institut Teoreticheskoi i Eksperimental'noi Fiziki and Institut Kosmicheskikh Issledovanii, Moscow, USSR
Akademiia Nauk SSSR, Institut Prikladnoi Matematiki; Gosudarstvennyi Komitet po Ispol'zovaniiu Atomnoi Energii, Institut Teoreticheskoi i Eksperimental'noi Fiziki, Moscow, USSR
AN SSSR, Institut Teoreticheskoi i Eksperimental'noi Fiziki, Moscow, USSR
Akademiia Nauk SSSR, Astronomicheskii Sovet, Moscow, USSR
A dynamical model of type I supernova atmosphere with the velocity gradient
A hydrodynamic model for asymmetric explosions of rapidly rotating collapsing supernovae with a toroidal atmosphere
A Hydrodynamic Model for Asymmetric Weak Explosion of Collapsing Supernovae with Rapid Initial Rotation
A numerical study of the stability of a rapidly rotating neutron star: axially symmetric model
A possible scenario of a supernova explosion as a result of the gravitational collapse of a massive stellar core
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