Zobrazeno 1 - 6
of 6
pro vyhledávání: '"D. V. Badmaev"'
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ce9a4c700fe3bcf633a15d28b4fe947c
https://doi.org/10.3103/s1062873823702313
https://doi.org/10.3103/s1062873823702313
Autor:
E. E. Kholupenko, D. V. Badmaev, A. S. Antonov, A. A. Bogdanov, A. M. Krassilchtchikov, D. O. Kuleshov, Yu. V. Tuboltsev, E. M. Khilkevich, Yu. V. Chichagov
Publikováno v:
Technical Physics. 67:80-103
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3e33e63677304ad4c06c0fb3eaebdeb2
https://doi.org/10.1134/s106378422201008x
https://doi.org/10.1134/s106378422201008x
Autor:
Yu. V. Tubol’tsev, E. E. Kholupenko, D. O. Kuleshov, D. V. Badmaev, Yu. V. Chichagov, A. S. Antonov, Andrey Bogdanov, E. M. Khil’kevich, A. M. Krassilchtchikov
Publikováno v:
Technical Physics. 65:886-895
Source and noise signals in a new camera of the TAIGA-IACT Cherenkov γ-ray telescope based on silicon photomultipliers (SiPM) have been simulated. It is shown that application of modern silicon photomultipliers as detecting elements of TAIGA-IACT (i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6b193496df2b70ba0bd818806e1a90a6
https://doi.org/10.1134/s1063784220060158
https://doi.org/10.1134/s1063784220060158
Young massive star clusters inhabit regions of star formation and play an essential role in the galactic evolution. They are sources of both thermal and non-thermal radiation, and they are effective cosmic ray accelerators. We present the 3D magnetoh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2e7dabf516c95cc4495e5ad2b962df1
Autor:
D V Badmaev, A M Bykov
Publikováno v:
Journal of Physics: Conference Series. 2103:012013
The fast stellar winds of massive stars, along with supernovae, determine the dynamics within the star-forming regions. Within a compact star cluster, counterpropagating supersonic MHD shock flows associated with winds and supernova remnants can prov
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::250effbb04de62dcccc039f58109efec
https://doi.org/10.1088/1742-6596/2103/1/012013
https://doi.org/10.1088/1742-6596/2103/1/012013
Autor:
D. V. Badmaev, A. M. Bykov
Publikováno v:
Journal of Physics: Conference Series. 1400:022033
Fast stellar winds of young massive stars and supernovae play an essential role in the evolution of the interstellar medium in the Milky Way. They dominate the dynamics of the active starforming regions in starburst galaxies and in particularly their
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8f0541330e4f551882d0ae5b9060b944
https://doi.org/10.1088/1742-6596/1400/2/022033
https://doi.org/10.1088/1742-6596/1400/2/022033