Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Institute of Astronomy Moscow, Russia
Institute of Astronomy of the Russian Acad. of Sci., Moscow;
Institute of Astronomy of the RAS, Moscow, Russia
INASAN, Russia
Illinois, University, Urbana
Akademiia Nauk SSSR, Astronomicheskii Sovet, Moscow, USSR
AN SSSR, Astronomicheskii Sovet, Moscow, USSR
Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya ul 48, Moscow, 119017 Russia
B'lgarska Akademiia na Naukite, Sektsiia po Astronomiia, Sofia, Bulgaria; Akademiia Nauk SSSR, Astronomicheskii Sovet, Moscow, USSR
Institute of Astronomy, Moscow, Russia
B'lgarska Akademiia na Naukite, Samostoiatelen Sektor po Astronomiia, Sofia, Bulgaria; Akademiia Nauk SSSR, Astronomicheskii Sovet, Moscow, USSR
B'lgarska Akademiia na Naukite Samostoiatelna Sektsiia po Astronomiia, Sofia, Bulgaria; Akademiia Nauk SSSR, Astronomicheskii Sovet, Moscow, USSR
AN SSSR, Astronomicheskii Sovet, Moscow, USSR; B'lgarska Akademiia na Naukite, Samostoiatelna Sektsiia Astronomiia, Sofia, Bulgaria
Institute of Astronomy RAS, Moscow 119017, Russia; Full Professor, Head of department, Department of Physics and Evolution of Stars, Institute of Astronomy RAS, 119017, Moscow, Russia;
Institute of Astronomy, Russian Academy of Sciences
Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya Str. 48, 109017 Moscow, Russia
RAN, Inst. Astronomii, Moscow, Russia
Rossiiskaia Akademiia Nauk, Institut Astronomii, Moscow, Russia
RAN, Inst. Astronomii
AN SSSR, Institut Astronomii, Moscow, USSR
Akademiia Nauk SSSR, Astronomicheskii Sovet, Moscow, USSR; Illinois University, Urbana, IL
Akademiia Nauk SSSR, Astronomicheskii Sovet, Moscow, USSR; Illinois, University, Urbana, IL
University of Illinois, Urbana, IL, US
AN SSSR, Astronomicheskii Sovet and Institut Prikladnoi Matematiki, Moscow, USSR
B'lgarska Akademiia na Naukite, Samostoiatelna Sektsiia po Astronomiia s Natsionalna Astronomicheska Observatoriia, Sofia, Bulgaria;
A dynamical model for the dusty envelope around the symbiotic nova PU Vulpeculae
A Dynamical Model for the Dusty Envelope around the Symbiotic Nova Pu-Vulpeculae
A hydrodynamical model of FG Sagittae pulsations
A Mechanism for the Oxygen and Iron Bimodal Radial Distribution Formation in the Disc of our Galaxy
A Model for the Population of Binary Stars in the Galaxy
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